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1. First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment

Author: Aalbers, J, Akerib, DS, Akerlof, CW, Al Musalhi, AK, Alder, F, Alqahtani, A, Alsum, SK, Amarasinghe, CS, Ames, A, Anderson, TJ, Angelides, N, Araújo, HM, Armstrong, JE, Arthurs, M, Azadi, S, Bailey, AJ, Baker, A, Balajthy, J, Balashov, S, Bang, J, Bargemann, JW, Barry, MJ, Barthel, J, Bauer, D, Baxter, A, Beattie, K, Belle, J, Beltrame, P, Bensinger, J, Benson, T, Bernard, EP, Bhatti, A, Biekert, A, Biesiadzinski, TP, Birch, HJ, Birrittella, B, Blockinger, GM, Boast, KE, Boxer, B, Bramante, R, Brew, CAJ, Brás, P, Buckley, JH, Bugaev, VV, Burdin, S, Busenitz, JK, Buuck, M, Cabrita, R, Carels, C, Carlsmith, DL, Carlson, B, Carmona-Benitez, MC, Cascella, M, Chan, C, Chawla, A, Chen, H, Cherwinka, JJ, Chott, NI, Cole, A, Coleman, J, Converse, MV, Cottle, A, Cox, G, Craddock, WW, Creaner, O, Curran, D, Currie, A, Cutter, JE, Dahl, CE, David, A, Davis, J, Davison, TJR, Delgaudio, J, Dey, S, de Viveiros, L, Dobi, A, Dobson, JEY, Druszkiewicz, E, Dushkin, A, Edberg, TK, Edwards, WR, Elnimr, MM, Emmet, WT, Eriksen, SR, Faham, CH, Fan, A, Fayer, S, Fearon, NM, Fiorucci, S, Flaecher, H, Ford, P, Francis, VB, Fraser, ED, Fruth, T, Gaitskell, RJ, Gantos, NJ, Garcia, D, Geffre, A, Gehman, VM, and Genovesi, J
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, LUX-ZEPLIN Collaboration, Mathematical Sciences, Engineering, General Physics, Mathematical sciences, Physical sciences
Abstract: The LUX-ZEPLIN experiment is a dark matter detector centered on a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility in Lead, South Dakota, USA. This Letter reports results from LUX-ZEPLIN's first search for weakly interacting massive particles (WIMPs) with an exposure of 60 live days using a fiducial mass of 5.5 t. A profile-likelihood ratio analysis shows the data to be consistent with a background-only hypothesis, setting new limits on spin-independent WIMP-nucleon, spin-dependent WIMP-neutron, and spin-dependent WIMP-proton cross sections for WIMP masses above 9 GeV/c^{2}. The most stringent limit is set for spin-independent scattering at 36 GeV/c^{2}, rejecting cross sections above 9.2×10^{-48} cm at the 90% confidence level.
Published: 2023

2. The LUX-ZEPLIN (LZ) experiment

Author: Akerib, DS, Akerlof, CW, Akimov, DY, Alquahtani, A, Alsum, SK, Anderson, TJ, Angelides, N, Araújo, HM, Arbuckle, A, Armstrong, JE, Arthurs, M, Auyeung, H, Bai, X, Bailey, AJ, Balajthy, J, Balashov, S, Bang, J, Barry, MJ, Barthel, J, Bauer, D, Bauer, P, Baxter, A, Belle, J, Beltrame, P, Bensinger, J, Benson, T, Bernard, EP, Bernstein, A, Bhatti, A, Biekert, A, Biesiadzinski, TP, Birrittella, B, Boast, KE, Bolozdynya, AI, Boulton, EM, Boxer, B, Bramante, R, Branson, S, Brás, P, Breidenbach, M, Buckley, JH, Bugaev, VV, Bunker, R, Burdin, S, Busenitz, JK, Campbell, JS, Carels, C, Carlsmith, DL, Carlson, B, Carmona-Benitez, MC, Cascella, M, Chan, C, Cherwinka, JJ, Chiller, AA, Chiller, C, Chott, NI, Cole, A, Coleman, J, Colling, D, Conley, RA, Cottle, A, Coughlen, R, Craddock, WW, Curran, D, Currie, A, Cutter, JE, da Cunha, JP, Dahl, CE, Dardin, S, Dasu, S, Davis, J, Davison, TJR, de Viveiros, L, Decheine, N, Dobi, A, Dobson, JEY, Druszkiewicz, E, Dushkin, A, Edberg, TK, Edwards, WR, Edwards, BN, Edwards, J, Elnimr, MM, Emmet, WT, Eriksen, SR, Faham, CH, Fan, A, Fayer, S, Fiorucci, S, Flaecher, H, Fogarty Florang, IM, Ford, P, Francis, VB, Froborg, F, Fruth, T, Gaitskell, RJ, Gantos, NJ, Garcia, D, Geffre, A, and Gehman, VM
Subjects: Dark matter detector, Liquid xenon, Time projection chamber, Underground, physics.ins-det, astro-ph.IM, hep-ex, Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Other Physical Sciences
Abstract: We describe the design and assembly of the LUX-ZEPLIN experiment, a direct detection search for cosmic WIMP dark matter particles. The centerpiece of the experiment is a large liquid xenon time projection chamber sensitive to low energy nuclear recoils. Rejection of backgrounds is enhanced by a Xe skin veto detector and by a liquid scintillator Outer Detector loaded with gadolinium for efficient neutron capture and tagging. LZ is located in the Davis Cavern at the 4850’ level of the Sanford Underground Research Facility in Lead, South Dakota, USA. We describe the major subsystems of the experiment and its key design features and requirements.
Published: 2020

3. Calibration, event reconstruction, data analysis, and limit calculation for the LUX dark matter experiment

Author: Akerib, DS, Alsum, S, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boulton, EM, Brás, P, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Currie, A, Cutter, JE, Davison, TJR, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fallon, SR, Fan, A, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Genovesi, J, Ghag, C, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Jacobsen, RG, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Manalaysay, A, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, JA, St. J. Murphy, A, Nehrkorn, C, Nelson, HN, Neves, F, O’Sullivan, K, Oliver-Mallory, KC, Palladino, KJ, Pease, EK, Reichhart, L, Rhyne, C, Shaw, S, Shutt, TA, Silva, C, Solmaz, M, Solovov, VN, Sorensen, P, Sumner, TJ, Szydagis, M, Taylor, DJ, Taylor, WC, Tennyson, BP, Terman, PA, Tiedt, DR, To, WH, Tripathi, M, Tvrznikova, L, Uvarov, S, Velan, V, Verbus, JR, Webb, RC, White, JT, Whitis, TJ, Witherell, MS, Wolfs, FLH, Xu, J, Yazdani, K, Young, SK, and Zhang, C
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Synchrotrons and Accelerators, Physical Sciences, Affordable and Clean Energy, physics.ins-det
Abstract: The LUX experiment has performed searches for dark-matter particles scattering elastically on xenon nuclei, leading to stringent upper limits on the nuclear scattering cross sections for dark matter. Here, for results derived from 1.4×104 kg days of target exposure in 2013, details of the calibration, event-reconstruction, modeling, and statistical tests that underlie the results are presented. Detector performance is characterized, including measured efficiencies, stability of response, position resolution, and discrimination between electron- and nuclear-recoil populations. Models are developed for the drift field, optical properties, background populations, the electron- and nuclear-recoil responses, and the absolute rate of low-energy background events. Innovations in the analysis include in situ measurement of the photomultipliers' response to xenon scintillation photons, verification of fiducial mass with a low-energy internal calibration source, and new empirical models for low-energy signal yield based on large-sample, in situ calibrations.
Published: 2018

4. Search for Neutrinoless Double-β Decay in Ge76 with the Majorana Demonstrator

Author: Aalseth, CE, Abgrall, N, Aguayo, E, Alvis, SI, Amman, M, Arnquist, IJ, Avignone, FT, Back, HO, Barabash, AS, Barbeau, PS, Barton, CJ, Barton, PJ, Bertrand, FE, Bode, T, Bos, B, Boswell, M, Bradley, AW, Brodzinski, RL, Brudanin, V, Busch, M, Buuck, M, Caldwell, AS, Caldwell, TS, Chan, Y-D, Christofferson, CD, Chu, P-H, Collar, JI, Combs, DC, Cooper, RJ, Cuesta, C, Detwiler, JA, Doe, PJ, Dunmore, JA, Efremenko, Yu, Ejiri, H, Elliott, SR, Fast, JE, Finnerty, P, Fraenkle, FM, Fu, Z, Fujikawa, BK, Fuller, E, Galindo-Uribarri, A, Gehman, VM, Gilliss, T, Giovanetti, GK, Goett, J, Green, MP, Gruszko, J, Guinn, IS, Guiseppe, VE, Hallin, AL, Haufe, CR, Hehn, L, Henning, R, Hoppe, EW, Hossbach, TW, Howe, MA, Jasinski, BR, Johnson, RA, Keeter, KJ, Kephart, JD, Kidd, MF, Knecht, A, Konovalov, SI, Kouzes, RT, LaFerriere, BD, Leon, J, Lesko, KT, Leviner, LE, Loach, JC, Lopez, AM, Luke, PN, MacMullin, J, MacMullin, S, Marino, MG, Martin, RD, Massarczyk, R, McDonald, AB, Mei, D-M, Meijer, SJ, Merriman, JH, Mertens, S, Miley, HS, Miller, ML, Myslik, J, Orrell, JL, O'Shaughnessy, C, Othman, G, Overman, NR, Perumpilly, G, Pettus, W, Phillips, DG, Poon, AWP, Pushkin, K, Radford, DC, Rager, J, Reeves, JH, Reine, AL, and Rielage, K
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Synchrotrons and Accelerators, Physical Sciences, Majorana Collaboration, nucl-ex, physics.ins-det, Mathematical Sciences, Engineering, General Physics, Mathematical sciences, Physical sciences
Abstract: The Majorana Collaboration is operating an array of high purity Ge detectors to search for neutrinoless double-β decay in ^{76}Ge. The Majorana Demonstrator comprises 44.1 kg of Ge detectors (29.7 kg enriched in ^{76}Ge) split between two modules contained in a low background shield at the Sanford Underground Research Facility in Lead, South Dakota. Here we present results from data taken during construction, commissioning, and the start of full operations. We achieve unprecedented energy resolution of 2.5 keV FWHM at Q_{ββ} and a very low background with no observed candidate events in 9.95 kg yr of enriched Ge exposure, resulting in a lower limit on the half-life of 1.9×10^{25} yr (90% C.L.). This result constrains the effective Majorana neutrino mass to below 240-520 meV, depending on the matrix elements used. In our experimental configuration with the lowest background, the background is 4.0_{-2.5}^{+3.1} counts/(FWHM t yr).
Published: 2018

5. Search for Neutrinoless Double-β Decay in ^{76}Ge with the Majorana Demonstrator.

Author: Aalseth, CE, Abgrall, N, Aguayo, E, Alvis, SI, Amman, M, Arnquist, IJ, Avignone, FT, Back, HO, Barabash, AS, Barbeau, PS, Barton, CJ, Barton, PJ, Bertrand, FE, Bode, T, Bos, B, Boswell, M, Bradley, AW, Brodzinski, RL, Brudanin, V, Busch, M, Buuck, M, Caldwell, AS, Caldwell, TS, Chan, Y-D, Christofferson, CD, Chu, P-H, Collar, JI, Combs, DC, Cooper, RJ, Cuesta, C, Detwiler, JA, Doe, PJ, Dunmore, JA, Efremenko, Yu, Ejiri, H, Elliott, SR, Fast, JE, Finnerty, P, Fraenkle, FM, Fu, Z, Fujikawa, BK, Fuller, E, Galindo-Uribarri, A, Gehman, VM, Gilliss, T, Giovanetti, GK, Goett, J, Green, MP, Gruszko, J, Guinn, IS, Guiseppe, VE, Hallin, AL, Haufe, CR, Hehn, L, Henning, R, Hoppe, EW, Hossbach, TW, Howe, MA, Jasinski, BR, Johnson, RA, Keeter, KJ, Kephart, JD, Kidd, MF, Knecht, A, Konovalov, SI, Kouzes, RT, LaFerriere, BD, Leon, J, Lesko, KT, Leviner, LE, Loach, JC, Lopez, AM, Luke, PN, MacMullin, J, MacMullin, S, Marino, MG, Martin, RD, Massarczyk, R, McDonald, AB, Mei, D-M, Meijer, SJ, Merriman, JH, Mertens, S, Miley, HS, Miller, ML, Myslik, J, Orrell, JL, O'Shaughnessy, C, Othman, G, Overman, NR, Perumpilly, G, Pettus, W, Phillips, DG, Poon, AWP, Pushkin, K, Radford, DC, Rager, J, Reeves, JH, Reine, AL, and Rielage, K
Subjects: Majorana Collaboration, nucl-ex, physics.ins-det, General Physics, Mathematical Sciences, Physical Sciences, Engineering
Abstract: The Majorana Collaboration is operating an array of high purity Ge detectors to search for neutrinoless double-β decay in ^{76}Ge. The Majorana Demonstrator comprises 44.1 kg of Ge detectors (29.7 kg enriched in ^{76}Ge) split between two modules contained in a low background shield at the Sanford Underground Research Facility in Lead, South Dakota. Here we present results from data taken during construction, commissioning, and the start of full operations. We achieve unprecedented energy resolution of 2.5 keV FWHM at Q_{ββ} and a very low background with no observed candidate events in 9.95 kg yr of enriched Ge exposure, resulting in a lower limit on the half-life of 1.9×10^{25} yr (90% C.L.). This result constrains the effective Majorana neutrino mass to below 240-520 meV, depending on the matrix elements used. In our experimental configuration with the lowest background, the background is 4.0_{-2.5}^{+3.1} counts/(FWHM t yr).
Published: 2018

6. Chromatographic separation of radioactive noble gases from xenon

Author: Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boulton, EM, Bramante, R, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chiller, AA, Chiller, C, Coffey, T, Currie, A, Cutter, JE, Davison, TJR, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Ihm, M, Jacobsen, RG, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Manalaysay, A, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, JA, Murphy, Nehrkorn, C, Nelson, HN, Neves, F, O’Sullivan, K, Oliver-Mallory, KC, Palladino, KJ, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Rhyne, C, Shaw, S, Shutt, TA, Silva, C, Solovov, VN, Sorensen, P, Stephenson, S, Sumner, TJ, Szydagis, M, Taylor, DJ, Taylor, W, Tennyson, BP, Terman, PA, Tiedt, DR, To, WH, Tripathi, M, Tvrznikova, L, Uvarov, S, Verbus, JR, Webb, RC, White, JT, Whitis, TJ, Witherell, MS, Wolfs, FLH, Yazdani, K, Young, SK, and Zhang, C
Subjects: Nuclear and Plasma Physics, Synchrotrons and Accelerators, Physical Sciences, Xenon, Krypton, Adsorption, Chromatography, Gas Separation, Dark Matter, physics.ins-det, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Nuclear & Particles Physics, Astronomical sciences, Particle and high energy physics
Abstract: The Large Underground Xenon (LUX) experiment operates at the Sanford Underground Research Facility to detect nuclear recoils from the hypothetical Weakly Interacting Massive Particles (WIMPs) on a liquid xenon target. Liquid xenon typically contains trace amounts of the noble radioactive isotopes 85Kr and 39Ar that are not removed by the in situ gas purification system. The decays of these isotopes at concentrations typical of research-grade xenon would be a dominant background for a WIMP search experiment. To remove these impurities from the liquid xenon, a chromatographic separation system based on adsorption on activated charcoal was built. 400 kg of xenon was processed, reducing the average concentration of krypton from 130 ppb to 3.5 ppt as measured by a cold-trap assisted mass spectroscopy system. A 50 kg batch spiked to 0.001 g/g of krypton was processed twice and reduced to an upper limit of 0.2 ppt.
Published: 2018

7. The MAJORANA DEMONSTRATOR calibration system

Author: Abgrall, N, Arnquist, IJ, Avignone III, FT, Barabash, AS, Bertrand, FE, Boswell, M, Bradley, AW, Brudanin, V, Busch, M, Buuck, M, Caldwell, TS, Christofferson, CD, Chu, PH, Cuesta, C, Detwiler, JA, Dunagan, C, Efremenko, Y, Ejiri, H, Elliott, SR, Fu, Z, Gehman, VM, Gilliss, T, Giovanetti, GK, Goett, J, Green, MP, Gruszko, J, Guinn, IS, Guiseppe, VE, Haufe, CR, Henning, R, Hoppe, EW, Howe, MA, Jasinski, BR, Keeter, KJ, Kidd, MF, Konovalov, SI, Kouzes, RT, Lopez, AM, MacMullin, J, Martin, RD, Massarczyk, R, Meijer, SJ, Mertens, S, Orrell, JL, O'Shaughnessy, C, Poon, AWP, Radford, DC, Rager, J, Reine, AL, Rielage, K, Robertson, RGH, Shanks, B, Shirchenko, M, Suriano, AM, Tedeschi, D, Trimble, JE, Varner, RL, Vasilyev, S, Vetter, K, Vorren, K, White, BR, Wilkerson, JF, Wiseman, C, Xu, W, Yu, CH, Yumatov, V, Zhitnikov, I, and Zhu, BX
Subjects: Neutrinoless double-beta decay, Germanium detector, Majorana, Detector calibration, physics.ins-det, nucl-ex, Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Other Physical Sciences
Abstract: The MAJORANA Collaboration is searching for the neutrinoless double-beta decay of the nucleus 76Ge. The MAJORANA DEMONSTRATOR is an array of germanium detectors deployed with the aim of implementing background reduction techniques suitable for a 1-ton 76Ge-based search. The ultra low-background conditions require regular calibrations to verify proper function of the detectors. Radioactive line sources can be deployed around the cryostats containing the detectors for regular energy calibrations. When measuring in low-background mode, these line sources have to be stored outside the shielding so they do not contribute to the background. The deployment and the retraction of the source are designed to be controlled by the data acquisition system and do not require any direct human interaction. In this paper, we detail the design requirements and implementation of the calibration apparatus, which provides the event rates needed to define the pulse-shape cuts and energy calibration used in the final analysis as well as data that can be compared to simulations.
Published: 2017

8. Identification of radiopure titanium for the LZ dark matter experiment and future rare event searches

Author: Akerib, DS, Akerlof, CW, Akimov, DY, Alsum, SK, Araújo, HM, Arnquist, IJ, Arthurs, M, Bai, X, Bailey, AJ, Balajthy, J, Balashov, S, Barry, MJ, Belle, J, Beltrame, P, Benson, T, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boast, KE, Bolozdynya, A, Boxer, B, Bramante, R, Brás, P, Buckley, JH, Bugaev, VV, Bunker, R, Burdin, S, Busenitz, JK, Carels, C, Carlsmith, DL, Carlson, B, Carmona-Benitez, MC, Chan, C, Cherwinka, JJ, Chiller, AA, Chiller, C, Cottle, A, Coughlen, R, Craddock, WW, Currie, A, Dahl, CE, Davison, TJR, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edberg, TK, Edwards, WR, Emmet, WT, Faham, CH, Fiorucci, S, Fruth, T, Gaitskell, RJ, Gantos, NJ, Gehman, VM, Gerhard, RM, Ghag, C, Gilchriese, MGD, Gomber, B, Hall, CR, Hans, S, Hanzel, K, Haselschwardt, SJ, Hertel, SA, Hillbrand, S, Hjemfelt, C, Hoff, MD, Holbrook, B, Holtom, E, Hoppe, EW, Hor, JYK, Horn, M, Huang, DQ, Hurteau, TW, Ignarra, CM, Jacobsen, RG, Ji, W, Kaboth, A, Kamdin, K, Kazkaz, K, Khaitan, D, Khazov, A, Khromov, AV, Konovalov, AM, Korolkova, EV, Koyuncu, M, Kraus, H, Krebs, HJ, Kudryavtsev, VA, Kumpan, AV, Kyre, S, Lee, C, Lee, HS, Lee, J, Leonard, DS, Leonard, R, Lesko, KT, Levy, C, Liao, FT, Lin, J, and Lindote, A
Subjects: physics.ins-det, hep-ex, Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics
Abstract: The LUX-ZEPLIN (LZ) experiment will search for dark matter particle interactions with a detector containing a total of 10 tonnes of liquid xenon within a double-vessel cryostat. The large mass and proximity of the cryostat to the active detector volume demand the use of material with extremely low intrinsic radioactivity. We report on the radioassay campaign conducted to identify suitable metals, the determination of factors limiting radiopure production, and the selection of titanium for construction of the LZ cryostat and other detector components. This titanium has been measured with activities of 238Ue < 1.6 mBq/kg, 238Ul < 0.09 mBq/kg, 232The=0.28±0.03 mBq/kg, 232Thl=0.25±0.02 mBq/kg, 40K < 0.54 mBq/kg, and 60Co < 0.02 mBq/kg (68% CL). Such low intrinsic activities, which are some of the lowest ever reported for titanium, enable its use for future dark matter and other rare event searches. Monte Carlo simulations have been performed to assess the expected background contribution from the LZ cryostat with this radioactivity. In 1,000 days of WIMP search exposure of a 5.6-tonne fiducial mass, the cryostat will contribute only a mean background of 0.160 ± 0.001(stat) ± 0.030(sys) counts.
Published: 2017

9. First Searches for Axions and Axionlike Particles with the LUX Experiment

Author: Akerib, DS, Alsum, S, Aquino, C, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boulton, EM, Brás, P, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chiller, AA, Chiller, C, Currie, A, Cutter, JE, Davison, TJR, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fallon, SR, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Jacobsen, RG, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Manalaysay, A, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, JA, Murphy, A St J, Nehrkorn, C, Nelson, HN, Neves, F, O'Sullivan, K, Oliver-Mallory, KC, Palladino, KJ, Pease, EK, Reichhart, L, Rhyne, C, Shaw, S, Shutt, TA, Silva, C, Solmaz, M, Solovov, VN, Sorensen, P, Stephenson, S, Sumner, TJ, Szydagis, M, Taylor, DJ, Taylor, WC, Tennyson, BP, Terman, PA, Tiedt, DR, To, WH, Tripathi, M, Tvrznikova, L, Uvarov, S, Velan, V, Verbus, JR, Webb, RC, White, JT, Whitis, TJ, Witherell, MS, Wolfs, FLH, Xu, J, Yazdani, K, and Young, SK
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, LUX Collaboration, astro-ph.CO, hep-ph, Mathematical Sciences, Engineering, General Physics, Mathematical sciences, Physical sciences
Abstract: The first searches for axions and axionlike particles with the Large Underground Xenon experiment are presented. Under the assumption of an axioelectric interaction in xenon, the coupling constant between axions and electrons g_{Ae} is tested using data collected in 2013 with an exposure totaling 95 live days ×118 kg. A double-sided, profile likelihood ratio statistic test excludes g_{Ae} larger than 3.5×10^{-12} (90% C.L.) for solar axions. Assuming the Dine-Fischler-Srednicki-Zhitnitsky theoretical description, the upper limit in coupling corresponds to an upper limit on axion mass of 0.12 eV/c^{2}, while for the Kim-Shifman-Vainshtein-Zhakharov description masses above 36.6 eV/c^{2} are excluded. For galactic axionlike particles, values of g_{Ae} larger than 4.2×10^{-13} are excluded for particle masses in the range 1-16 keV/c^{2}. These are the most stringent constraints to date for these interactions.
Published: 2017

10. Limits on Spin-Dependent WIMP-Nucleon Cross Section Obtained from the Complete LUX Exposure

Author: Akerib, DS, Alsum, S, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boulton, EM, Brás, P, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chiller, AA, Chiller, C, Currie, A, Cutter, JE, Davison, TJR, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fallon, SR, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Jacobsen, RG, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Manalaysay, A, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, JA, Murphy, A St J, Nehrkorn, C, Nelson, HN, Neves, F, O'Sullivan, K, Oliver-Mallory, KC, Palladino, KJ, Pease, EK, Reichhart, L, Rhyne, C, Shaw, S, Shutt, TA, Silva, C, Solmaz, M, Solovov, VN, Sorensen, P, Stephenson, S, Sumner, TJ, Szydagis, M, Taylor, DJ, Taylor, WC, Tennyson, BP, Terman, PA, Tiedt, DR, To, WH, Tripathi, M, Tvrznikova, L, Uvarov, S, Velan, V, Verbus, JR, Webb, RC, White, JT, Whitis, TJ, Witherell, MS, Wolfs, FLH, Xu, J, Yazdani, K, Young, SK, and Zhang, C
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, LUX Collaboration, astro-ph.CO, Mathematical Sciences, Engineering, General Physics, Mathematical sciences, Physical sciences
Abstract: We present experimental constraints on the spin-dependent WIMP-nucleon elastic cross sections from the total 129.5 kg yr exposure acquired by the Large Underground Xenon experiment (LUX), operating at the Sanford Underground Research Facility in Lead, South Dakota (USA). A profile likelihood ratio analysis allows 90% C.L. upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of σ_{n}=1.6×10^{-41} cm^{2} (σ_{p}=5×10^{-40} cm^{2}) at 35 GeV c^{-2}, almost a sixfold improvement over the previous LUX spin-dependent results. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date.
Published: 2017

11. LUX-ZEPLIN (LZ) Technical Design Report

Author: Mount, BJ, Hans, S, Rosero, R, Yeh, M, Chan, C, Gaitskell, RJ, Huang, DQ, Makkinje, J, Malling, DC, Pangilinan, M, Rhyne, CA, Taylor, WC, Verbus, JR, Kim, YD, Lee, HS, Lee, J, Leonard, DS, Li, J, Belle, J, Cottle, A, Lippincott, WH, Markley, DJ, Martin, TJ, Sarychev, M, Tope, TE, Utes, M, Wang, R, Young, I, Araújo, HM, Bailey, AJ, Bauer, D, Colling, D, Currie, A, Fayer, S, Froborg, F, Greenwood, S, Jones, WG, Kasey, V, Khaleeq, M, Olcina, I, Paredes, B López, Richards, A, Sumner, TJ, Tomás, A, Vacheret, A, Brás, P, Lindote, A, Lopes, MI, Neves, F, Rodrigues, JP, Silva, C, Solovov, VN, Barry, MJ, Cole, A, Dobi, A, Edwards, WR, Faham, CH, Fiorucci, S, Gantos, NJ, Gehman, VM, Gilchriese, MGD, Hanzel, K, Hoff, MD, Kamdin, K, Lesko, KT, McConnell, CT, O'Sullivan, K, Oliver-Mallory, KC, Patton, SJ, Saba, JS, Sorensen, P, Thomas, KJ, Tull, CE, Waldron, WL, Witherell, MS, Bernstein, A, Kazkaz, K, Xu, J, Akimov, D Yu, Bolozdynya, AI, Khromov, AV, Konovalov, AM, Kumpan, AV, Sosnovtsev, VV, Dahl, CE, Temples, D, Carmona-Benitez, MC, Viveiros, L de, Akerib, DS, Auyeung, H, Biesiadzinski, TP, Breidenbach, M, Bramante, R, Conley, R, Craddock, WW, Fan, A, Hau, A, Ignarra, CM, Ji, W, and Krebs, HJ
Subjects: physics.ins-det, astro-ph.IM, hep-ex
Abstract: In this Technical Design Report (TDR) we describe the LZ detector to be builtat the Sanford Underground Research Facility (SURF). The LZ dark matterexperiment is designed to achieve sensitivity to a WIMP-nucleonspin-independent cross section of three times ten to the negative forty-eighthsquare centimeters.
Published: 2017

12. Signal yields, energy resolution, and recombination fluctuations in liquid xenon

Author: Akerib, DS, Alsum, S, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boulton, EM, Bramante, R, Brás, P, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chiller, AA, Chiller, C, Currie, A, Cutter, JE, Davison, TJR, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Ihm, M, Jacobsen, RG, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Manalaysay, A, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, DM, Mock, J, Moongweluwan, M, Morad, JA, Murphy, ASJ, Nehrkorn, C, Nelson, HN, Neves, F, O'Sullivan, K, Oliver-Mallory, KC, Palladino, KJ, Pease, EK, Phelps, P, Reichhart, L, Rhyne, C, Shaw, S, Shutt, TA, Silva, C, Solmaz, M, Solovov, VN, Sorensen, P, Stephenson, S, Sumner, TJ, Szydagis, M, Taylor, DJ, Taylor, WC, Tennyson, BP, Terman, PA, Tiedt, DR, To, WH, Tripathi, M, Tvrznikova, L, Uvarov, S, Verbus, JR, Webb, RC, White, JT, Whitis, TJ, Witherell, MS, Wolfs, FLH, Xu, J, Yazdani, K, and Young, SK
Subjects: physics.ins-det, hep-ex
Abstract: This work presents an analysis of monoenergetic electronic recoil peaks in the dark-matter-search and calibration data from the first underground science run of the Large Underground Xenon (LUX) detector. Liquid xenon charge and light yields for electronic recoil energies between 5.2 and 661.7 keV are measured, as well as the energy resolution for the LUX detector at those same energies. Additionally, there is an interpretation of existing measurements and descriptions of electron-ion recombination fluctuations in liquid xenon as limiting cases of a more general liquid xenon recombination fluctuation model. Measurements of the standard deviation of these fluctuations at monoenergetic electronic recoil peaks exhibit a linear dependence on the number of ions for energy deposits up to 661.7 keV, consistent with previous LUX measurements between 2 and 16 keV with H3. We highlight similarities in liquid xenon recombination for electronic and nuclear recoils with a comparison of recombination fluctuations measured with low-energy calibration data.
Published: 2017

13. Results from a Search for Dark Matter in the Complete LUX Exposure

Author: Akerib, DS, Alsum, S, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boulton, EM, Bramante, R, Brás, P, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chiller, AA, Chiller, C, Currie, A, Cutter, JE, Davison, TJR, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Ihm, M, Jacobsen, RG, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Manalaysay, A, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, JA, Murphy, A St J, Nehrkorn, C, Nelson, HN, Neves, F, O'Sullivan, K, Oliver-Mallory, KC, Palladino, KJ, Pease, EK, Phelps, P, Reichhart, L, Rhyne, C, Shaw, S, Shutt, TA, Silva, C, Solmaz, M, Solovov, VN, Sorensen, P, Stephenson, S, Sumner, TJ, Szydagis, M, Taylor, DJ, Taylor, WC, Tennyson, BP, Terman, PA, Tiedt, DR, To, WH, Tripathi, M, Tvrznikova, L, Uvarov, S, Verbus, JR, Webb, RC, White, JT, Whitis, TJ, Witherell, MS, Wolfs, FLH, Xu, J, Yazdani, K, and Young, SK
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, LUX Collaboration, astro-ph.CO, astro-ph.IM, hep-ex, physics.ins-det, Mathematical Sciences, Engineering, General Physics, Mathematical sciences, Physical sciences
Abstract: We report constraints on spin-independent weakly interacting massive particle (WIMP)-nucleon scattering using a 3.35×10^{4} kg day exposure of the Large Underground Xenon (LUX) experiment. A dual-phase xenon time projection chamber with 250 kg of active mass is operated at the Sanford Underground Research Facility under Lead, South Dakota (USA). With roughly fourfold improvement in sensitivity for high WIMP masses relative to our previous results, this search yields no evidence of WIMP nuclear recoils. At a WIMP mass of 50 GeV c^{-2}, WIMP-nucleon spin-independent cross sections above 2.2×10^{-46} cm^{2} are excluded at the 90% confidence level. When combined with the previously reported LUX exposure, this exclusion strengthens to 1.1×10^{-46} cm^{2} at 50 GeV c^{-2}.
Published: 2017

14. The Majorana Demonstrator radioassay program

Author: Abgrall, N, Arnquist, IJ, Avignone, FT, Back, HO, Barabash, AS, Bertrand, FE, Boswell, M, Bradley, AW, Brudanin, V, Busch, M, Buuck, M, Byram, D, Caldwell, AS, Chan, YD, Christofferson, CD, Chu, PH, Cuesta, C, Detwiler, JA, Dunmore, JA, Efremenko, Y, Ejiri, H, Elliott, SR, Finnerty, P, Galindo-Uribarri, A, Gehman, VM, Gilliss, T, Giovanetti, GK, Goett, J, Green, MP, Gruszko, J, Guinn, IS, Guiseppe, VE, Henning, R, Hoppe, EW, Howard, S, Howe, MA, Jasinski, BR, Johnson, RA, Keeter, KJ, Kidd, MF, Kochetov, O, Konovalov, SI, Kouzes, RT, LaFerriere, BD, Leon, J, Loach, JC, Macmullin, J, Macmullin, S, Martin, RD, Massarczyk, R, Meijer, S, Mertens, S, Miller, ML, Orrell, JL, O'Shaughnessy, C, Overman, NR, Poon, AWP, Pushkin, K, Radford, DC, Rager, J, Rielage, K, Robertson, RGH, Romero-Romero, E, Ronquest, MC, Schubert, AG, Shanks, B, Shirchenko, M, Snavely, KJ, Snyder, N, Steele, D, Suriano, AM, Tedeschi, D, Trimble, JE, Varner, RL, Vasilyev, S, Vetter, K, Vorren, K, White, BR, Wilkerson, JF, Wiseman, C, Xu, W, Yakushev, E, Yu, CH, Yumatov, V, and Zhitnikov, I
Subjects: Radiopurity, Trace analysis, Neutron activation analysis, Mass spectrometry, Mass spectroscopy, Germanium counting, Low background, Double beta decay, MAJORANA, physics.ins-det, hep-ex, nucl-ex, Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Other Physical Sciences
Abstract: The Majorana collaboration is constructing the Majorana Demonstrator at the Sanford Underground Research Facility at the Homestake gold mine, in Lead, SD. The apparatus will use Ge detectors, enriched in isotope 76Ge, to demonstrate the feasibility of a large-scale Ge detector experiment to search for neutrinoless double beta decay. The long half-life of this postulated process requires that the apparatus be extremely low in radioactive isotopes whose decays may produce backgrounds to the search. The radioassay program conducted by the collaboration to ensure that the materials comprising the apparatus are sufficiently pure is described. The resulting measurements from gamma-ray counting, neutron activation and mass spectroscopy of the radioactive-isotope contamination for the materials studied for use in the detector are reported. We interpret these numbers in the context of the expected background for the experiment.
Published: 2016

15. FPGA-based trigger system for the LUX dark matter experiment

Author: Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boulton, EM, Bradley, A, Bramante, R, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Currie, A, Cutter, JE, Davison, TJR, De Viveiros, L, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Ihm, M, Jacobsen, RG, Ji, W, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Manalaysay, AG, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, DM, Mock, J, Moongweluwan, M, Morad, JA, Murphy, ASJ, Nehrkorn, C, Nelson, HN, Neves, F, O'Sullivan, K, Oliver-Mallory, KC, Ott, RA, Palladino, KJ, Pangilinan, M, Pease, EK, Phelps, P, Reichhart, L, Rhyne, C, Shaw, S, Shutt, TA, Silva, C, Skulski, W, Solovov, VN, Sorensen, P, Stephenson, S, Sumner, TJ, Szydagis, M, Taylor, DJ, Taylor, W, Tennyson, BP, Terman, PA, Tiedt, DR, To, WH, Tripathi, M, Tvrznikova, L, Uvarov, S, Verbus, JR, Webb, RC, White, JT, Whitis, TJ, Witherell, MS, Wolfs, FLH, and Yin, J
Subjects: Trigger, Dark matter detectors, DSP, FPGA, DAQ, Baseline subtraction, physics.ins-det, Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Other Physical Sciences
Abstract: LUX is a two-phase (liquid/gas) xenon time projection chamber designed to detect nuclear recoils resulting from interactions with dark matter particles. Signals from the detector are processed with an FPGA-based digital trigger system that analyzes the incoming data in real-time, with just a few microsecond latency. The system enables first pass selection of events of interest based on their pulse shape characteristics and 3D localization of the interactions. It has been shown to be >99% efficient in triggering on S2 signals induced by only few extracted liquid electrons. It is continuously and reliably operating since its full underground deployment in early 2013. This document is an overview of the systems capabilities, its inner workings, and its performance.
Published: 2016

16. Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX Data

Author: Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boulton, EM, Bradley, A, Bramante, R, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Currie, A, Cutter, JE, Davison, TJR, de Viveiros, L, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Ihm, M, Jacobsen, RG, Ji, W, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Manalaysay, A, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, JA, Murphy, A St J, Nehrkorn, C, Nelson, HN, Neves, F, O'Sullivan, K, Oliver-Mallory, KC, Ott, RA, Palladino, KJ, Pangilinan, M, Pease, EK, Phelps, P, Reichhart, L, Rhyne, C, Shaw, S, Shutt, TA, Silva, C, Solovov, VN, Sorensen, P, Stephenson, S, Sumner, TJ, Szydagis, M, Taylor, DJ, Taylor, W, Tennyson, BP, Terman, PA, Tiedt, DR, To, WH, Tripathi, M, Tvrznikova, L, Uvarov, S, Verbus, JR, Webb, RC, White, JT, Whitis, TJ, Witherell, MS, Wolfs, FLH, Yazdani, K, and Young, SK
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, LUX Collaboration, astro-ph.CO, astro-ph.IM, hep-ex, physics.ins-det, Mathematical Sciences, Engineering, General Physics, Mathematical sciences, Physical sciences
Abstract: We present constraints on weakly interacting massive particles (WIMP)-nucleus scattering from the 2013 data of the Large Underground Xenon dark matter experiment, including 1.4×10^{4} kg day of search exposure. This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV. Sensitivity, especially to low-mass WIMPs, is enhanced compared to our previous results which modeled the signal only above a 3 keV minimum energy. Under standard dark matter halo assumptions and in the mass range above 4 GeV c^{-2}, these new results give the most stringent direct limits on the spin-independent WIMP-nucleon cross section. The 90% C.L. upper limit has a minimum of 0.6 zb at 33 GeV c^{-2} WIMP mass.
Published: 2016

17. Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment

Author: Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boulton, EM, Bradley, A, Bramante, R, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Currie, A, Cutter, JE, Davison, TJR, de Viveiros, L, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Ihm, M, Jacobsen, RG, Ji, W, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Manalaysay, A, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, JA, Murphy, A St J, Nehrkorn, C, Nelson, HN, Neves, F, O'Sullivan, K, Oliver-Mallory, KC, Ott, RA, Palladino, KJ, Pangilinan, M, Pease, EK, Phelps, P, Reichhart, L, Rhyne, C, Shaw, S, Shutt, TA, Silva, C, Solovov, VN, Sorensen, P, Stephenson, S, Sumner, TJ, Szydagis, M, Taylor, DJ, Taylor, W, Tennyson, BP, Terman, PA, Tiedt, DR, To, WH, Tripathi, M, Tvrznikova, L, Uvarov, S, Verbus, JR, Webb, RC, White, JT, Whitis, TJ, Witherell, MS, Wolfs, FLH, Yazdani, K, and Young, SK
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Synchrotrons and Accelerators, Physical Sciences, LUX Collaboration, hep-ex, hep-ph, Mathematical Sciences, Engineering, General Physics, Mathematical sciences, Physical sciences
Abstract: We present experimental constraints on the spin-dependent WIMP (weakly interacting massive particle)-nucleon elastic cross sections from LUX data acquired in 2013. LUX is a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), which is designed to observe the recoil signature of galactic WIMPs scattering from xenon nuclei. A profile likelihood ratio analysis of 1.4×10^{4} kg day of fiducial exposure allows 90% C.L. upper limits to be set on the WIMP-neutron (WIMP-proton) cross section of σ_{n}=9.4×10^{-41} cm^{2} (σ_{p}=2.9×10^{-39} cm^{2}) at 33 GeV/c^{2}. The spin-dependent WIMP-neutron limit is the most sensitive constraint to date.
Published: 2016

18. Tritium calibration of the LUX dark matter experiment

Author: Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boulton, EM, Bradley, A, Bramante, R, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Currie, A, Cutter, JE, Davison, TJR, De Viveiros, L, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Ihm, M, Jacobsen, RG, Ji, W, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Manalaysay, AG, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, DM, Mock, J, Moongweluwan, M, Morad, JA, Murphy, ASJ, Nehrkorn, C, Nelson, HN, Neves, F, O'Sullivan, K, Oliver-Mallory, KC, Ott, RA, Palladino, KJ, Pangilinan, M, Pease, EK, Phelps, P, Reichhart, L, Rhyne, C, Shaw, S, Shutt, TA, Silva, C, Solovov, VN, Sorensen, P, Stephenson, S, Sumner, TJ, Szydagis, M, Taylor, DJ, Taylor, W, Tennyson, BP, Terman, PA, Tiedt, DR, To, WH, Tripathi, M, Tvrznikova, L, Uvarov, S, Verbus, JR, Webb, RC, White, JT, Whitis, TJ, Witherell, MS, Wolfs, FLH, Young, SK, and Zhang, C
Subjects: physics.ins-det, astro-ph.IM, hep-ex
Abstract: We present measurements of the electron-recoil (ER) response of the LUX dark matter detector based upon 170 000 highly pure and spatially uniform tritium decays. We reconstruct the tritium energy spectrum using the combined energy model and find good agreement with expectations. We report the average charge and light yields of ER events in liquid xenon at 180 and 105 V/cm and compare the results to the NEST model. We also measure the mean charge recombination fraction and its fluctuations, and we investigate the location and width of the LUX ER band. These results provide input to a reanalysis of the LUX run 3 weakly interacting massive particle search.
Published: 2016

19. First Results of the LUX Dark Matter Experiment

Author: Carmona-Benitez, MC, Collaboration, LUX, Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, E, Bernstein, A, Bradley, A, Byram, D, Cahn, SB, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Currie, A, de Viveiros, L, Dobi, A, Dobson, J, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hanhardt, M, Haselschwardt, S, Hertel, SA, Horn, M, Huang, DQ, Ihm, M, Jacobsen, RG, Kazkaz, K, Knoche, R, Larsen, NA, Lee, C, Lenardo, B, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Manalaysay, A, Mannino, R, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J, Murphy, Nehrkorn, C, Nelson, H, Neves, F, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Solovov, VN, Sorensen, P, O'Sullivan, K, Sumner, TJ, Szydagis, M, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Tvrznikova, L, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, Witherell, MS, Wolfs, FLH, Woods, M, and Zhang, C
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, dark matter, WIMP, liquid xenon, time projection chamber
Abstract: LUX (Large Underground Xenon) is a dark matter direct detection experiment deployed at the 4850' level of the Sanford Underground Research Facility (SURF) in Lead, SD, operating a 370 kg dual-phase xenon TPC. Results of the first WIMP search run were presented in late 2013, for the analysis of 85.3 live-days with a fiducial volume of 118 kg, taken during the period of April to August 2013. The experiment exhibited a sensitivity to spin-independent WIMP-nucleon elastic scattering with a minimum upper limit on the cross section of 7.6×10-46cm2 at a WIMP mass of 33 GeV/c2, becoming the world's leading WIMP search result, in conflict with several previous claimed hints of discovery.
Published: 2016

20. First proof of topological signature in the high pressure xenon gas TPC with electroluminescence amplification for the NEXT experiment

Author: The NEXT collaboration, Ferrario, P, Laing, A, López-March, N, Gómez-Cadenas, JJ, Álvarez, V, Azevedo, CDR, Borges, FIG, Cárcel, S, Cebrián, S, Cervera, A, Conde, CAN, Dafni, T, Díaz, J, Diesburg, M, Esteve, R, Fernandes, LMP, Ferreira, AL, Freitas, EDC, Gehman, VM, Goldschmidt, A, González-Díaz, D, Gutiérrez, RM, Hauptman, J, Henriques, CAO, Hernando Morata, JA, Irastorza, IG, Labarga, L, Lebrun, P, Liubarsky, I, Lorca, D, Losada, M, Luzón, G, Marí, A, Martín-Albo, J, Martínez-Lema, G, Martínez, A, Miller, T, Monrabal, F, Monserrate, M, Monteiro, CMB, Mora, FJ, Moutinho, LM, Muñoz Vidal, J, Nebot-Guinot, M, Novella, P, Nygren, D, Para, A, Pérez, J, Pérez Aparicio, JL, Querol, M, Renner, J, Ripoll, L, Rodríguez, J, Santos, FP, dos Santos, JMF, Serra, L, Shuman, D, Simón, A, Sofka, C, Sorel, M, Toledo, JF, Torrent, J, Tsamalaidze, Z, Veloso, JFCA, Villar, JA, Webb, R, White, JT, Yahlali, N, and Yepes-Ramírez, H
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, Dark Matter, Double Beta Decay, Mathematical Physics, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Mathematical physics, Nuclear and plasma physics, Particle and high energy physics
Abstract: The NEXT experiment aims to observe the neutrinoless double beta decay of 136Xe in a high-pressure xenon gas TPC using electroluminescence (EL) to amplify the signal from ionization. One of the main advantages of this technology is the possibility to reconstruct the topology of events with energies close to Qββ. This paper presents the first demonstration that the topology provides extra handles to reject background events using data obtained with the NEXT-DEMO prototype. Single electrons resulting from the interactions of 22Na 1275 keV gammas and electronpositron pairs produced by conversions of gammas from the 228Th decay chain were used to represent the background and the signal in a double beta decay. These data were used to develop algorithms for the reconstruction of tracks and the identification of the energy deposited at the end-points, providing an extra background rejection factor of 24.3 ± 1.4 (stat.)%, while maintaining an efficiency of 66.7 ± 1.% for signal events.[Figure not available: see fulltext.]
Published: 2016

21. First proof of topological signature in the high pressure xenon gas TPC with electroluminescence amplification for the NEXT experiment

Author: Ferrario, P, Laing, A, López-March, N, Gómez-Cadenas, JJ, Álvarez, V, Azevedo, CDR, Borges, FIG, Cárcel, S, Cebrián, S, Cervera, A, Conde, CAN, Dafni, T, Díaz, J, Diesburg, M, Esteve, R, Fernandes, LMP, Ferreira, AL, Freitas, EDC, Gehman, VM, Goldschmidt, A, González-Díaz, D, Gutiérrez, RM, Hauptman, J, Henriques, CAO, Hernando Morata, JA, Irastorza, IG, Labarga, L, Lebrun, P, Liubarsky, I, Lorca, D, Losada, M, Luzón, G, Marí, A, Martín-Albo, J, Martínez-Lema, G, Martínez, A, Miller, T, Monrabal, F, Monserrate, M, Monteiro, CMB, Mora, FJ, Moutinho, LM, Muñoz Vidal, J, Nebot-Guinot, M, Novella, P, Nygren, D, Para, A, Pérez, J, Pérez Aparicio, JL, Querol, M, Renner, J, Ripoll, L, Rodríguez, J, Santos, FP, dos Santos, JMF, Serra, L, Shuman, D, Simón, A, Sofka, C, Sorel, M, Toledo, JF, Torrent, J, Tsamalaidze, Z, Veloso, JFCA, Villar, JA, Webb, R, White, JT, Yahlali, N, and Yepes-Ramírez, H
Subjects: Dark Matter, Double Beta Decay, Nuclear & Particles Physics, Mathematical Sciences, Physical Sciences, Mathematical Physics, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Atomic, Molecular, Nuclear, Particle and Plasma Physics
Abstract: The NEXT experiment aims to observe the neutrinoless double beta decay of 136Xe in a high-pressure xenon gas TPC using electroluminescence (EL) to amplify the signal from ionization. One of the main advantages of this technology is the possibility to reconstruct the topology of events with energies close to Qββ. This paper presents the first demonstration that the topology provides extra handles to reject background events using data obtained with the NEXT-DEMO prototype. Single electrons resulting from the interactions of 22Na 1275 keV gammas and electronpositron pairs produced by conversions of gammas from the 228Th decay chain were used to represent the background and the signal in a double beta decay. These data were used to develop algorithms for the reconstruction of tracks and the identification of the energy deposited at the end-points, providing an extra background rejection factor of 24.3 ± 1.4 (stat.)%, while maintaining an efficiency of 66.7 ± 1.% for signal events.[Figure not available: see fulltext.]
Published: 2016

22. Results from the LUX dark matter experiment

Author: Horn, M, Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Bernard, E, Bernstein, A, Bradley, A, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Currie, A, De Viveiros, L, Dobi, A, Dobson, J, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hanhardt, M, Haselschwardt, S, Hertel, SA, Huang, DQ, Ihm, M, Jacobsen, RG, Kazkaz, K, Knoche, R, Larsen, NA, Lee, C, Lenardo, B, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Mannino, R, McKinsey, DN, Mei, DM, Mock, J, Moongweluwan, M, Morad, J, Murphy, ASJ, Nehrkorn, C, Nelson, H, Neves, F, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Solovov, VN, Sorensen, P, O'Sullivan, K, Sumner, TJ, Szydagis, M, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, Witherell, MS, Wolfs, FLH, Woods, M, and Zhang, C
Subjects: Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Other Physical Sciences, Nuclear & Particles Physics, Nuclear and plasma physics
Abstract: The LUX (Large Underground Xenon) experiment aims at the direct detection of dark matter particles via their collisions with xenon nuclei. The 370 kg two-phase liquid xenon time projection chamber measures simultaneously the scintillation and ionization from interactions in the target. The ratio of these two signals provides very good discrimination between potential nuclear recoil and electronic recoil signals to search for WIMP-nucleon scattering. The LUX detector operates at the Sanford Underground Research Facility (Lead, South Dakota, USA) since February 2013. First results were presented in late 2013 setting the world's most stringent limits on WIMP-nucleon scattering cross-sections over a wide range of WIMP masses. A 300 day run beginning in 2014 will further improve the sensitivity and new calibration techniques will reduce systematics for the WIMP signal search.
Published: 2015

23. Results from the LUX dark matter experiment

Author: Horn, Markus, Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Bernard, E, Bernstein, A, Bradley, A, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Currie, A, de Viveiros, L, Dobi, A, Dobson, J, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hanhardt, M, Haselschwardt, S, Hertel, SA, Huang, DQ, Ihm, M, Jacobsen, RG, Kazkaz, K, Knoche, R, Larsen, NA, Lee, C, Lenardo, B, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Mannino, R, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J, Murphy, Nehrkorn, C, Nelson, H, Neves, F, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Solovov, VN, Sorensen, P, O׳Sullivan, K, Sumner, TJ, Szydagis, M, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, Witherell, MS, Wolfs, FLH, Woods, M, Zhang, C, and Collaboration, On behalf of the LUX
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Synchrotrons and Accelerators, Physical Sciences, Dark matter, WIMP, Liquid xenon, Time projection chamber, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Other Physical Sciences, Nuclear & Particles Physics, Nuclear and plasma physics
Abstract: © 2014 Elsevier B.V. The LUX (Large Underground Xenon) experiment aims at the direct detection of dark matter particles via their collisions with xenon nuclei. The 370. kg two-phase liquid xenon time projection chamber measures simultaneously the scintillation and ionization from interactions in the target. The ratio of these two signals provides very good discrimination between potential nuclear recoil and electronic recoil signals to search for WIMP-nucleon scattering. The LUX detector operates at the Sanford Underground Research Facility (Lead, South Dakota, USA) since February 2013. First results were presented in late 2013 setting the world's most stringent limits on WIMP-nucleon scattering cross-sections over a wide range of WIMP masses. A 300 day run beginning in 2014 will further improve the sensitivity and new calibration techniques will reduce systematics for the WIMP signal search.
Published: 2015

24. Radiogenic and muon-induced backgrounds in the LUX dark matter detector

Author: Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Bernard, E, Bernstein, A, Bradley, A, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Coffey, T, Currie, A, de Viveiros, L, Dobi, A, Dobson, J, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hertel, SA, Horn, M, Huang, DQ, Ihm, M, Jacobsen, RG, Kazkaz, K, Knoche, R, Larsen, NA, Lee, C, Lindote, A, Lopes, MI, Malling, DC, Mannino, R, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J, Murphy, Nehrkorn, C, Nelson, H, Neves, F, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Solovov, VN, Sorensen, P, O’Sullivan, K, Sumner, TJ, Szydagis, M, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, Witherell, MS, Wolfs, FLH, Woods, M, and Zhang, C
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, LUX, Dark matter, Radioactive background, Material screening, Simulation, astro-ph.IM, physics.ins-det, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Nuclear & Particles Physics, Astronomical sciences, Particle and high energy physics
Abstract: The Large Underground Xenon (LUX) dark matter experiment aims to detect rare low-energy interactions from Weakly Interacting Massive Particles (WIMPs). The radiogenic backgrounds in the LUX detector have been measured and compared with Monte Carlo simulation. Measurements of LUX high-energy data have provided direct constraints on all background sources contributing to the background model. The expected background rate from the background model for the 85.3 day WIMP search run is (2.6±0.2stat±0.4sys) ×10-3 events keVee-1kg-1day-1 in a 118 kg fiducial volume. The observed background rate is (3.6±0.4 stat)×10-3 events keVee-1kg-1day- 1, consistent with model projections. The expectation for the radiogenic background in a subsequent one-year run is presented. © 2014 Elsevier B.V. All rights reserved.
Published: 2015

25. Radon-related Backgrounds in the LUX Dark Matter Search

Author: Bradley, A, Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Bernard, E, Bernstein, A, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Coffey, T, Currie, A, de Viveiros, L, Dobi, A, Dobson, J, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hertel, SA, Horn, M, Huang, DQ, Ihm, M, Jacobsen, RG, Kazkaz, K, Knoche, R, Larsen, NA, Lee, C, Lindote, A, Lopes, MI, Malling, DC, Mannino, R, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J, Murphy, A St J, Nehrkorn, C, Nelson, H, Neves, F, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Solovov, VN, Sorensen, P, O'Sullivan, K, Sumner, TJ, Szydagis, M, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, Witherell, MS, Wolfs, FLH, Woods, M, and Zhang, C
Subjects: dark matter, liquid noble detectors, xenon, radon, background characterization
Abstract: The LUX detector is currently in operation at the Davis Campus at the 4850' level of the Sanford Underground Research Facility (SURF) in Lead, SD to directly search for WIMP dark matter. Knowing the type and rate of backgrounds is critical in a rare, low energy event search, and LUX was designed, constructed, and deployed to mitigate backgrounds, both internal and external. An important internal background are decays of radon and its daughters. These consist of alpha decays, which are easily tagged and are a tracer of certain backgrounds, and beta decays, some of which are not as readily tagged and present a background for the WIMP search. We report on studies of alpha decay and discuss implications for the WIMP search.
Published: 2015

26. The LUX Experiment

Author: Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Bernard, E, Bernstein, A, Bradley, A, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Coffey, T, Currie, A, de Viveiros, L, Dobi, A, Dobson, J, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hertel, SA, Horn, M, Huang, DQ, Ihm, M, Jacobsen, RG, Kazkaz, K, Knoche, R, Larsen, NA, Lee, C, Lindote, A, Lopes, MI, Malling, DC, Mannino, R, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J, Murphy, A St J, Nehrkorn, C, Nelson, H, Neves, F, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Solovov, VN, Sorensen, P, O'Sullivan, K, Sumner, TJ, Szydagis, M, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, Witherell, MS, Wolfs, FLH, Woods, M, and Zhang, C
Subjects: Liquid xenon detectors, Dark matter, WIMP, Direct detection
Abstract: We present the status and prospects of the LUX experiment, which employs approximately 300 kg of two-phase xenon to search for WIMP dark matter interactions. The LUX detector was commissioned at the surface laboratory of the Sanford Underground Research Facility in Lead, SD, between December 2011 and February 2012 and the detector has been operating underground since January, 2013. These proceedings review the results of the commissioning run as well as the status of underground data-taking through the summer of 2013.
Published: 2015

27. First Results from the LUX Dark Matter Experiment at the Sanford Underground Research Facility

Author: Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Bedikian, S, Bernard, E, Bernstein, A, Bolozdynya, A, Bradley, A, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Clark, K, Coffey, T, Currie, A, Curioni, A, Dazeley, S, de Viveiros, L, Dobi, A, Dobson, J, Dragowsky, EM, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hanhardt, M, Hertel, SA, Horn, M, Huang, DQ, Ihm, M, Jacobsen, RG, Kastens, L, Kazkaz, K, Knoche, R, Kyre, S, Lander, R, Larsen, NA, Lee, C, Leonard, DS, Lesko, KT, Lindote, A, Lopes, MI, Lyashenko, A, Malling, DC, Mannino, R, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J, Morii, M, Murphy, A St J, Nehrkorn, C, Nelson, H, Neves, F, Nikkel, JA, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Skulski, W, Sofka, CJ, Solovov, VN, Sorensen, P, Stiegler, T, O'Sullivan, K, Sumner, TJ, Svoboda, R, Sweany, M, Szydagis, M, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, White, D, Witherell, MS, Wlasenko, M, and Wolfs, FLH
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, LUX Collaboration, astro-ph.CO, astro-ph.IM, hep-ex, physics.ins-det, Mathematical Sciences, Engineering, General Physics, Mathematical sciences, Physical sciences
Abstract: The Large Underground Xenon (LUX) experiment is a dual-phase xenon time-projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota). The LUX cryostat was filled for the first time in the underground laboratory in February 2013. We report results of the first WIMP search data set, taken during the period from April to August 2013, presenting the analysis of 85.3 live days of data with a fiducial volume of 118 kg. A profile-likelihood analysis technique shows our data to be consistent with the background-only hypothesis, allowing 90% confidence limits to be set on spin-independent WIMP-nucleon elastic scattering with a minimum upper limit on the cross section of 7.6 × 10(-46) cm(2) at a WIMP mass of 33 GeV/c(2). We find that the LUX data are in disagreement with low-mass WIMP signal interpretations of the results from several recent direct detection experiments.
Published: 2014

28. A Detailed Look at the First Results from the Large Underground Xenon (LUX) Dark Matter Experiment

Author: Szydagis, M, Akerib, DS, Araujo, HM, Bai, X, Bailey, AJ, Balajthy, J, Bernard, E, Bernstein, A, Bradley, A, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Coffey, T, Currie, A, Viveiros, L de, Dobi, A, Dobson, J, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hertel, SA, Horn, M, Huang, DQ, Ihm, M, Jacobsen, RG, Kazkaz, K, Knoche, R, Larsen, NA, Lee, C, Lindote, A, Lopes, MI, Malling, DC, Mannino, R, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J, Murphy, A St J, Nehrkorn, C, Nelson, H, Neves, F, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Solovov, VN, Sorensen, P, O'Sullivan, K, Sumner, T, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, Witherell, MS, Wolfs, FLH, Woods, M, and Zhang, C
Subjects: hep-ex, astro-ph.CO, astro-ph.IM, physics.ins-det
Abstract: LUX, the world's largest dual-phase xenon time-projection chamber, with afiducial target mass of 118 kg and 10,091 kg-days of exposure thus far, iscurrently the most sensitive direct dark matter search experiment. The initialnull-result limit on the spin-independent WIMP-nucleon scattering cross-sectionwas released in October 2013, with a primary scintillation threshold of 2 phe,roughly 3 keVnr for LUX. The detector has been deployed at the SanfordUnderground Research Facility (SURF) in Lead, South Dakota, and is the firstexperiment to achieve a limit on the WIMP cross-section lower than $10^{-45}$cm$^{2}$. Here we present a more in-depth discussion of the novel energy scaleemployed to better understand the nuclear recoil light and charge yields, andof the calibration sources, including the new internal tritium source. We foundthe LUX data to be in conflict with low-mass WIMP signal interpretations ofother results.
Published: 2014

29. Present Status and Future Perspectives of the NEXT Experiment

Author: Cadenas, JJ Gómez, Álvarez, V, Borges, FIG, Cárcel, S, Castel, J, Cebrián, S, Cervera, A, Conde, CAN, Dafni, T, Dias, THVT, Díaz, J, Egorov, M, Esteve, R, Evtoukhovitch, P, Fernandes, LMP, Ferrario, P, Ferreira, AL, Freitas, EDC, Gehman, VM, Gil, A, Goldschmidt, A, Gómez, H, González-Díaz, D, Gutiérrez, RM, Hauptman, J, Morata, JA Hernando, Herrera, DC, Iguaz, FJ, Irastorza, IG, Jinete, MA, Labarga, L, Laing, A, Liubarsky, I, Lopes, JAM, Lorca, D, Losada, M, Luzón, G, Marí, A, Martín-Albo, J, Martínez, A, Miller, T, Moiseenko, A, Monrabal, F, Monserrate, M, Monteiro, CMB, Mora, FJ, Moutinho, LM, Vidal, J Muñoz, da Luz, H Natal, Navarro, G, Nebot-Guinot, M, Nygren, D, Oliveira, CAB, Palma, R, Pérez, Javier, Pérez-Aparicio, JL, Renner, J, Ripoll, L, Rodríguez, A, Rodríguez, J, Santos, FP, dos Santos, JMF, Seguí, L, Serra, L, Shuman, D, Simón, A, Sofka, C, Sorel, M, Toledo, JF, Tomás, A, Torrent, J, Tsamalaidze, Z, Veloso, JFCA, Villar, JA, Webb, R, White, J, and Yahlali, N
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, physics.ins-det, Mathematical Sciences, Mathematical sciences, Physical sciences
Abstract: NEXT is an experiment dedicated to neutrinoless double beta decay searches in xenon. The detector is a TPC, holding 100 kg of high-pressure xenon enriched in the 136Xe isotope. It is under construction in the Laboratorio Subterráneo de Canfranc in Spain, and it will begin operations in 2015. The NEXT detector concept provides an energy resolutionbetter than 1% FWHM and a topological signal that can be used to reduce the background. Furthermore, the NEXT technology can be extrapolated to a 1 ton-scale experiment. © 2014 J. J. Gómez Cadenas et al.
Published: 2014

30. Direct search for dark matter with two-phase xenon detectors: Current status of LUX and plans for LZ

Author: Akerib, DS, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Bernard, E, Bernstein, A, Bradley, A, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Coffey, T, Currie, A, De Viveiros, L, Dobi, A, Dobson, J, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hertel, SA, Horn, M, Huang, DQ, Ihm, M, Jacobsen, RG, Kazkaz, K, Knoche, R, Larsen, NA, Lee, C, Lenardo, B, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Man-Nino, R, McKinsey, DN, Mei, DM, Mock, J, Moongweluwan, M, Morad, J, Murphy, ASJ, Nehrkorn, C, Nelson, H, Neves, F, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Solovov, VN, Sorensen, P, O'Sullivan, K, Sumner, TJ, Szydagis, M, Tay-Lor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, Witherell, MS, Wolfs, FLH, Woods, M, and Zhang, C
Abstract: The search for dark matter reaches back generations and remains one of the most compelling endeavors in the hunt for physics beyond the Standard Model. Experiments attempting to directly detect WIMP dark matter have made re-markable progress in increasing sensitivity to elastic scattering of WIMPs on nuclei. The LUX experiment is a 370-kg, two-phase, xenon TPC currently running at SURF, 4850 feet below Lead, SD. LUX recently completed its first science run and was sensitive to spin independent WIMP scattering at cross sections below 10-45 cm2 for WIMP masses of approximately 20 to 80 GeV. Preparations for the final science run of LUX are currently underway, with final results expected in 2015. We will present results from and current status of the LUX experiment, as well as plans for a follow-on, multi-ton-scale xenon experiment at SURF.
Published: 2014

31. Results from the LUX dark matter experiment

Author: Horn, M, Akerib, DS, Arau jo, HM, Bai, X, Bailey, AJ, Balajthy, J, Bernard, E, Bernstein, A, Bradley, A, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Currie, A, de Viveiros, L, Dobi, A, Dobson, J, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hanhardt, M, Haselschwardt, S, Hertel, SA, Huang, DQ, Ihm, M, Jacobsen, RG, Kazkaz, K, Knoche, R, Larsen, NA, Lee, C, Lenardo, B, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Mannino, R, McKinsey, DN, Mei, DM, Mock, J, Moongweluwan, M, Morad, J, Murphy, ASJ, Nehrkorn, C, Nelson, H, Neves, F, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Solovov, VN, Sorensen, P, O'Sullivan, K, Sumner, TJ, Szydagis, M, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, Witherell, MS, Wolfs, FLH, Woods, M, and Zhang, C
Subjects: Dark matter, WIMP, Liquid xenon, Time projection chamber, Nuclear & Particles Physics, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Other Physical Sciences
Abstract: © 2014 Elsevier B.V. The LUX (Large Underground Xenon) experiment aims at the direct detection of dark matter particles via their collisions with xenon nuclei. The 370. kg two-phase liquid xenon time projection chamber measures simultaneously the scintillation and ionization from interactions in the target. The ratio of these two signals provides very good discrimination between potential nuclear recoil and electronic recoil signals to search for WIMP-nucleon scattering. The LUX detector operates at the Sanford Underground Research Facility (Lead, South Dakota, USA) since February 2013. First results were presented in late 2013 setting the world's most stringent limits on WIMP-nucleon scattering cross-sections over a wide range of WIMP masses. A 300 day run beginning in 2014 will further improve the sensitivity and new calibration techniques will reduce systematics for the WIMP signal search.
Published: 2014

32. Present status and future perspectives of the NEXT experiment

Author: Gómez Cadenas, JJ, Álvarez, V, Borges, FIG, Cárcel, S, Castel, J, Cebrián, S, Cervera, A, Conde, CAN, Dafni, T, Dias, THVT, Díaz, J, Egorov, M, Esteve, R, Evtoukhovitch, P, Fernandes, LMP, Ferrario, P, Ferreira, AL, Freitas, EDC, Gehman, VM, Gil, A, Goldschmidt, A, Gómez, H, González-Díaz, D, Gutiérrez, RM, Hauptman, J, Hernando Morata, JA, Herrera, DC, Iguaz, FJ, Irastorza, IG, Jinete, MA, Labarga, L, Laing, A, Liubarsky, I, Lopes, JAM, Lorca, D, Losada, M, Luzón, G, Marí, A, Martín-Albo, J, Martínez, A, Miller, T, Moiseenko, A, Monrabal, F, Monserrate, M, Monteiro, CMB, Mora, FJ, Moutinho, LM, Muñoz Vidal, J, Natal Da Luz, H, Navarro, G, Nebot-Guinot, M, Nygren, D, Oliveira, CAB, Palma, R, Pérez, J, Pérez-Aparicio, JL, Renner, J, Ripoll, L, Rodríguez, A, Rodríguez, J, Santos, FP, Santos, JMFD, Seguí, L, Serra, L, Shuman, D, Simón, A, Sofka, C, Sorel, M, Toledo, JF, Tomás, A, Torrent, J, Tsamalaidze, Z, Veloso, JFCA, Villar, JA, Webb, R, White, J, and Yahlali, N
Subjects: physics.ins-det, Mathematical Sciences, Physical Sciences
Abstract: NEXT is an experiment dedicated to neutrinoless double beta decay searches in xenon. The detector is a TPC, holding 100 kg of high-pressure xenon enriched in the 136Xe isotope. It is under construction in the Laboratorio Subterráneo de Canfranc in Spain, and it will begin operations in 2015. The NEXT detector concept provides an energy resolutionbetter than 1% FWHM and a topological signal that can be used to reduce the background. Furthermore, the NEXT technology can be extrapolated to a 1 ton-scale experiment. © 2014 J. J. Gómez Cadenas et al.
Published: 2014

33. Astroparticle physics with a customized low-background broad energy Germanium detector

Author: Aalseth, CE, Amman, M, Avignone, FT, Back, HO, Barabash, AS, Barbeau, PS, Bergevin, M, Bertrand, FE, Boswell, M, Brudanin, V, Bugg, W, Burritt, TH, Busch, M, Capps, G, Chan, Y-D, Collar, JI, Cooper, RJ, Creswick, R, Detwiler, JA, Diaz, J, Doe, PJ, Efremenko, Yu, Egorov, V, Ejiri, H, Elliott, SR, Ely, J, Esterline, J, Farach, H, Fast, JE, Fields, N, Finnerty, P, Fujikawa, B, Fuller, E, Gehman, VM, Giovanetti, GK, Guiseppe, VE, Gusey, K, Hallin, AL, Harper, GC, Hazama, R, Henning, R, Hime, A, Hoppe, EW, Hossbach, TW, Howe, MA, Johnson, RA, Keeter, KJ, Keillor, M, Keller, C, Kephart, JD, Kidd, MF, Knecht, A, Kochetov, O, Konovalov, SI, Kouzes, RT, Leviner, L, Loach, JC, Luke, PN, MacMullin, S, Marino, MG, Martin, RD, Mei, D-M, Miley, HS, Miller, ML, Mizouni, L, Meyers, AW, Nomachi, M, Orrell, JL, Peterson, D, Phillips, DG, Poon, AWP, Prior, G, Qian, J, Radford, DC, Rielage, K, Robertson, RGH, Rodriguez, L, Rykaczewski, KP, Salazar, H, Schubert, AG, Shima, T, Shirchenko, M, Steele, D, Strain, J, Swift, G, Thomas, K, Timkin, V, Tornow, W, Van Wechel, TD, Vanyushin, I, Varner, RL, Vetter, K, Wilkerson, JF, Wolfe, BA, Xiang, W, Yakushev, E, Yaver, H, Young, AR, Yu, C-H, and Yumatov, V
Subjects: Nuclear and Plasma Physics, Particle and High Energy Physics, Synchrotrons and Accelerators, Physical Sciences, Low-background, Germanium detector, Dark matter, Neutrino experiments, Neutrino properties, nucl-ex, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Other Physical Sciences, Nuclear & Particles Physics, Nuclear and plasma physics
Abstract: The Majorana Collaboration is building the Majorana Demonstrator, a 60 kg array of high purity germanium detectors housed in an ultra-low background shield at the Sanford Underground Laboratory in Lead, SD. The Majorana Demonstrator will search for neutrinoless double-beta decay of 76Ge while demonstrating the feasibility of a tonne-scale experiment. It may also carry out a dark matter search in the 110 GeV/c2 mass range. We have found that customized Broad Energy Germanium (BEGe) detectors produced by Canberra have several desirable features for a neutrinoless double-beta decay experiment, including low electronic noise, excellent pulse shape analysis capabilities, and simple fabrication. We have deployed a customized BEGe, the Majorana Low-Background BEGe at Kimballton (MALBEK), in a low-background cryostat and shield at the Kimballton Underground Research Facility in Virginia. This paper will focus on the detector characteristics and measurements that can be performed with such a radiation detector in a low-background environment. © 2010 Elsevier B.V.
Published: 2011

34. Depth Requirements for a Tonne-scale 76Ge Neutrinoless Double-beta Decay Experiment

Author: Collaboration, The MAJORANA, Aguayo, E, III, FT Avignone, Back, HO, Barabash, AS, Bergevin, M, Bertrand, FE, Boswell, M, Brudanin, V, Busch, M, Chan, Y-D, Christofferson, CD, Collar, JI, Combs, DC, Cooper, RJ, Detwiler, JA, Doe, PJ, Efremenko, Yu, Egorov, V, Ejiri, H, Elliott, SR, Esterline, J, Fast, JE, Fields, N, Finnerty, P, Fraenkle, FM, Gehman, VM, Giovanetti, GK, Green, MP, Guiseppe, VE, Gusey, K, Hallin, AL, Hazama, R, Henning, R, Hime, A, Hoppe, EW, Horton, M, Howard, S, Howe, MA, Johnson, RA, Keeter, KJ, Keillor, ME, Keller, C, Kephart, JD, Kidd, MF, Knecht, A, Kochetov, O, Konovalov, SI, Kouzes, RT, LaFerriere, BD, LaRoque, BH, Leon, J, Leviner, LE, Loach, JC, MacMullin, S, Marino, MG, Martin, RD, Mei, D-M, Merriman, JH, Miller, ML, Mizouni, L, Nomachi, M, Orrell, JL, Overman, NR, II, DG Phillips, Poon, AWP, Perumpilly, G, Prior, G, Radford, DC, Rielage, K, Robertson, RGH, Ronquest, MC, Schubert, AG, Shima, T, Shirchenko, M, Snavely, KJ, Sobolev, V, Steele, D, Strain, J, Thomas, K, Timkin, V, Tornow, W, Vanyushin, I, Varner, RL, Vetter, K, Vorren, K, Wilkerson, JF, Wolfe, BA, Yakushev, E, Young, AR, Yu, C-H, Yumatov, V, and Zhang, C
Subjects: nucl-ex
Abstract: Neutrinoless double-beta decay experiments can potentially determine theMajorana or Dirac nature of the neutrino, and aid in understanding the neutrinoabsolute mass scale and hierarchy. Future 76Ge-based searches target ahalf-life sensitivity of >10^27 y to explore the inverted neutrino masshierarchy. Reaching this sensitivity will require a background rate of ~5200 mwe is required for atonne-scale experiment with a compact shield similar to the planned 40-kgMAJORANA DEMONSTRATOR. The required overburden is highly dependent on thechosen shielding configuration and could be relaxed significantly if, forexample, a liquid cryogen and water shield, or an active neutron shield wereemployed. Operation of the MAJORANA DEMONSTRATOR and GERDA detectors will serveto reduce the uncertainties on cosmic-ray background rates and will impact thechoice of shielding style and location for a future tonne-scale experiment. 4/2013: The peer review process revealed that one of the veto rejectionfactors (the factor-of-4 described on p12) needs to be better established. Ourreevaluation of this parameter to date has not yielded strong support for thevalue stated in the manuscript, and we require further study to develop a solidestimate. This further study will supersede the work described in thismanuscript, and may or may not lead to the same conclusion regarding the ~>5200mwe requirement for future tonne-scale 76Ge neutrinoless double beta decayexperiments.
Published: 2011

35. A Detailed Look at the First Results from the Large Underground Xenon (LUX) Dark Matter Experiment

Author: Szydagis, M, Akerib, DS, Araujo, HM, Bai, X, Bailey, AJ, Balajthy, J, Bernard, E, Bernstein, A, Bradley, A, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Coffey, T, Currie, A, Viveiros, L de, Dobi, A, Dobson, J, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Flores, C, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, C, Hertel, SA, Horn, M, Huang, DQ, Ihm, M, Jacobsen, RG, Kazkaz, K, Knoche, R, Larsen, NA, Lee, C, Lindote, A, Lopes, MI, Malling, DC, Mannino, R, McKinsey, DN, Mei, D-M, Mock, J, Moongweluwan, M, Morad, J, Murphy, A St J, Nehrkorn, C, Nelson, H, Neves, F, Ott, RA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Reichhart, L, Shutt, T, Silva, C, Solovov, VN, Sorensen, P, O'Sullivan, K, Sumner, T, Taylor, D, Tennyson, B, Tiedt, DR, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, JT, Witherell, MS, Wolfs, FLH, Woods, M, and Zhang, C
Subjects: High Energy Physics - Experiment (hep-ex), Physics - Instrumentation and Detectors, Cosmology and Nongalactic Astrophysics (astro-ph.CO), hep-ex, astro-ph.CO, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), physics.ins-det, High Energy Physics - Experiment, Astrophysics - Cosmology and Nongalactic Astrophysics, astro-ph.IM
Abstract: LUX, the world's largest dual-phase xenon time-projection chamber, with a fiducial target mass of 118 kg and 10,091 kg-days of exposure thus far, is currently the most sensitive direct dark matter search experiment. The initial null-result limit on the spin-independent WIMP-nucleon scattering cross-section was released in October 2013, with a primary scintillation threshold of 2 phe, roughly 3 keVnr for LUX. The detector has been deployed at the Sanford Underground Research Facility (SURF) in Lead, South Dakota, and is the first experiment to achieve a limit on the WIMP cross-section lower than $10^{-45}$ cm$^{2}$. Here we present a more in-depth discussion of the novel energy scale employed to better understand the nuclear recoil light and charge yields, and of the calibration sources, including the new internal tritium source. We found the LUX data to be in conflict with low-mass WIMP signal interpretations of other results., Comment: 16 pages, 3 figures, to appear in the proceedings of The 10th International Symposium on Cosmology and Particle Astrophysics (CosPA2013); fixed author list and added info on new calibration
Published: 2018

36. Search for Neutrinoless Double- β Decay in Ge 76 with the Majorana Demonstrator

Author: Aalseth, CE, Abgrall, N, Aguayo, E, Alvis, SI, Amman, M, Arnquist, IJ, Avignone, FT, Back, HO, Barabash, AS, Barbeau, PS, Barton, CJ, Barton, PJ, Bertrand, FE, Bode, T, Bos, B, Boswell, M, Bradley, AW, Brodzinski, RL, Brudanin, V, Busch, M, Buuck, M, Caldwell, AS, Caldwell, TS, Chan, YD, Christofferson, CD, Chu, PH, Collar, JI, Combs, DC, Cooper, RJ, Cuesta, C, Detwiler, JA, Doe, PJ, Dunmore, JA, Efremenko, Y, Ejiri, H, Elliott, SR, Fast, JE, Finnerty, P, Fraenkle, FM, Fu, Z, Fujikawa, BK, Fuller, E, Galindo-Uribarri, A, Gehman, VM, Gilliss, T, Giovanetti, GK, Goett, J, Green, MP, Gruszko, J, Guinn, IS, Guiseppe, VE, Hallin, AL, Haufe, CR, Hehn, L, Henning, R, Hoppe, EW, Hossbach, TW, Howe, MA, Jasinski, BR, Johnson, RA, Keeter, KJ, Kephart, JD, Kidd, MF, and Knecht, A
Subjects: nucl-ex, physics.ins-det
Abstract: © 2018 American Physical Society. The Majorana Collaboration is operating an array of high purity Ge detectors to search for neutrinoless double-β decay in Ge76. The Majorana Demonstrator comprises 44.1 kg of Ge detectors (29.7 kg enriched in Ge76) split between two modules contained in a low background shield at the Sanford Underground Research Facility in Lead, South Dakota. Here we present results from data taken during construction, commissioning, and the start of full operations. We achieve unprecedented energy resolution of 2.5 keV FWHM at Qββ and a very low background with no observed candidate events in 9.95 kg yr of enriched Ge exposure, resulting in a lower limit on the half-life of 1.9×1025 yr (90% C.L.). This result constrains the effective Majorana neutrino mass to below 240-520 meV, depending on the matrix elements used. In our experimental configuration with the lowest background, the background is 4.0-2.5+3.1 counts/(FWHM t yr).
Published: 2018

37. Search for Zero-Neutrino Double Beta Decay in 76Ge with the Majorana Demonstrator

Author: Aalseth, CE, Abgrall, N, Aguayo, E, Alvis, SI, Amman, M, Arnquist, IJ, III, FTA, Back, HO, Barabash, AS, Barbeau, PS, Barton, CJ, Barton, PJ, Bertrand, FE, Bode, T, Bos, B, Boswell, M, Brodzinski, RL, Bradley, AW, Brudanin, V, Busch, M, Buuck, M, Caldwell, AS, Caldwell, TS, Chan, Y-D, Christofferson, CD, Chu, P-H, Collar, JI, Combs, DC, Cooper, RJ, Cuesta, C, Detwiler, JA, Doe, PJ, Dunmore, JA, Efremenko, Y, Ejiri, H, Elliott, SR, Fast, JE, Finnerty, P, Fraenkle, FM, Fu, Z, Fujikawa, BK, Fuller, E, Galindo-Uribarri, A, Gehman, VM, Gilliss, T, Giovanetti, GK, Goett, J, Green, MP, Gruszko, J, Guinn, IS, Guiseppe, VE, Hallin, AL, Haufe, CR, Hehn, L, Henning, R, Hoppe, EW, Hossbach, TW, Howe, MA, Jasinski, BR, Johnson, RA, Keeter, KJ, Kephart, JD, Kidd, MF, Knecht, A, Konovalov, SI, Kouzes, RT, Lesko, KT, LaFerriere, BD, Leon, J, Leviner, LE, Loach, JC, Lopez, AM, Luke, PN, MacMullin, J, MacMullin, S, Marino, MG, Martin, RD, Massarczyk, R, McDonald, AB, Mei, D-M, Meijer, SJ, Merriman, JH, Mertens, S, Miley, HS, Miller, ML, Myslik, J, Orrell, JL, O'Shaughnessy, C, Othman, G, Overman, NR, Pettus, W, II, DGP, Poon, AWP, Perumpilly, G, Pushkin, K, Radford, DC, Rager, J, Reeves, JH, Reine, AL, Rielage, K, Robertson, RGH, Ronquest, MC, Ruof, NW, Schubert, AG, Shanks, B, Shirchenko, M, Snavely, KJ, Snyder, N, Steele, D, Suriano, AM, Tedeschi, D, Tornow, W, Trimble, JE, Varner, RL, Vasilyev, S, Vetter, K, Vorren, K, White, BR, Wilkerson, JF, Wiseman, C, Xu, W, Yakushev, E, Yaver, H, Young, AR, Yu, C-H, Yumatov, V, Zhitnikov, I, Zhu, BX, Zimmermann, S, Aalseth, CE, Abgrall, N, Aguayo, E, Alvis, SI, Amman, M, Arnquist, IJ, III, FTA, Back, HO, Barabash, AS, Barbeau, PS, Barton, CJ, Barton, PJ, Bertrand, FE, Bode, T, Bos, B, Boswell, M, Brodzinski, RL, Bradley, AW, Brudanin, V, Busch, M, Buuck, M, Caldwell, AS, Caldwell, TS, Chan, Y-D, Christofferson, CD, Chu, P-H, Collar, JI, Combs, DC, Cooper, RJ, Cuesta, C, Detwiler, JA, Doe, PJ, Dunmore, JA, Efremenko, Y, Ejiri, H, Elliott, SR, Fast, JE, Finnerty, P, Fraenkle, FM, Fu, Z, Fujikawa, BK, Fuller, E, Galindo-Uribarri, A, Gehman, VM, Gilliss, T, Giovanetti, GK, Goett, J, Green, MP, Gruszko, J, Guinn, IS, Guiseppe, VE, Hallin, AL, Haufe, CR, Hehn, L, Henning, R, Hoppe, EW, Hossbach, TW, Howe, MA, Jasinski, BR, Johnson, RA, Keeter, KJ, Kephart, JD, Kidd, MF, Knecht, A, Konovalov, SI, Kouzes, RT, Lesko, KT, LaFerriere, BD, Leon, J, Leviner, LE, Loach, JC, Lopez, AM, Luke, PN, MacMullin, J, MacMullin, S, Marino, MG, Martin, RD, Massarczyk, R, McDonald, AB, Mei, D-M, Meijer, SJ, Merriman, JH, Mertens, S, Miley, HS, Miller, ML, Myslik, J, Orrell, JL, O'Shaughnessy, C, Othman, G, Overman, NR, Pettus, W, II, DGP, Poon, AWP, Perumpilly, G, Pushkin, K, Radford, DC, Rager, J, Reeves, JH, Reine, AL, Rielage, K, Robertson, RGH, Ronquest, MC, Ruof, NW, Schubert, AG, Shanks, B, Shirchenko, M, Snavely, KJ, Snyder, N, Steele, D, Suriano, AM, Tedeschi, D, Tornow, W, Trimble, JE, Varner, RL, Vasilyev, S, Vetter, K, Vorren, K, White, BR, Wilkerson, JF, Wiseman, C, Xu, W, Yakushev, E, Yaver, H, Young, AR, Yu, C-H, Yumatov, V, Zhitnikov, I, Zhu, BX, and Zimmermann, S
Abstract: The \MJ\ Collaboration is operating an array of high purity Ge detectors to search for neutrinoless double-beta decay in $^{76}$Ge. The \MJ\ \DEM\ comprises 44.1~kg of Ge detectors (29.7 kg enriched in $^{76}$Ge) split between two modules contained in a low background shield at the Sanford Underground Research Facility in Lead, South Dakota. Here we present results from data taken during construction, commissioning, and the start of full operations. We achieve unprecedented energy resolution of 2.5 keV FWHM at \qval\ and a very low background with no observed candidate events in 10 kg yr of enriched Ge exposure, resulting in a lower limit on the half-life of $1.9\times10^{25}$ yr (90\% CL). This result constrains the effective Majorana neutrino mass to below 240 to 520 meV, depending on the matrix elements used. In our experimental configuration with the lowest background, the background is $4.0_{-2.5}^{+3.1}$ counts/(FWHM t yr).
Published: 2018

38. Low-energy (0.7-74 keV) nuclear recoil calibration of the LUX dark matter experiment using D-D neutron scattering kinematics

Author: Collaboration, LUX, Akerib, DS, Alsum, S, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Whitis, TJ, Witherell, MS, Wolfs, FLH, Xu, J, Yazdani, K, Young, SK, Zhang, C, Boulton, EM, Bradley, A, Bramante, R, Brás, P, Byram, D, Cahn, SB, Carmona-Benitez, MC, Chan, C, Chapman, JJ, Chiller, AA, Chiller, C, Currie, A, Cutter, JE, Davison, TJR, Viveiros, LD, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edwards, BN, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gehman, VM, Ghag, C, Gibson, KR, Gilchriese, MGD, Hall, CR, Hanhardt, M, Haselschwardt, SJ, Hertel, SA, Hogan, DP, Horn, M, Huang, DQ, Ignarra, CM, Ihm, M, Jacobsen, RG, Ji, W, Kamdin, K, Kazkaz, K, Khaitan, D, Knoche, R, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Lindote, A, Lopes, MI, Malling, DC, Manalaysay, A, Mannino, RL, Marzioni, MF, McKinsey, DN, Mei, DM, Mock, J, Moongweluwan, M, Morad, JA, Murphy, ASJ, Nehrkorn, C, Nelson, HN, Neves, F, O'Sullivan, K, Oliver-Mallory, KC, Palladino, KJ, Pangilinan, M, Pease, EK, Phelps, P, Reichhart, L, Rhyne, CA, Shaw, S, Shutt, TA, Silva, C, Solmaz, M, Solovov, VN, Sorensen, P, Stephenson, S, Sumner, TJ, Szydagis, M, Taylor, DJ, Taylor, WC, Tennyson, BP, Terman, PA, Tiedt, DR, To, WH, Tripathi, M, Tvrznikova, L, Uvarov, S, Verbus, JR, Webb, RC, and White, JT
Subjects: Physics::Instrumentation and Detectors, hep-ex, Astrophysics::Instrumentation and Methods for Astrophysics, Nuclear Experiment, physics.ins-det, astro-ph.IM
Abstract: The Large Underground Xenon (LUX) experiment is a dual-phase liquid xenon time projection chamber (TPC) operating at the Sanford Underground Research Facility in Lead, South Dakota. A calibration of nuclear recoils in liquid xenon was performed $\textit{in situ}$ in the LUX detector using a collimated beam of mono-energetic 2.45 MeV neutrons produced by a deuterium-deuterium (D-D) fusion source. The nuclear recoil energy from the first neutron scatter in the TPC was reconstructed using the measured scattering angle defined by double-scatter neutron events within the active xenon volume. We measured the absolute charge ($Q_{y}$) and light ($L_{y}$) yields at an average electric field of 180 V/cm for nuclear recoil energies spanning 0.7 to 74 keV and 1.1 to 74 keV, respectively. This calibration of the nuclear recoil signal yields will permit the further refinement of liquid xenon nuclear recoil signal models and, importantly for dark matter searches, clearly demonstrates measured ionization and scintillation signals in this medium at recoil energies down to $\mathcal{O}$(1 keV).
Published: 2016

39. Long-Baseline Neutrino Facility (LBNF) and Deep Underground Neutrino Experiment (DUNE) Conceptual Design Report, Volume 4 The DUNE Detectors at LBNF

Author: Acciarri, R, Acero, MA, Adamowski, M, Adams, C, Adamson, P, Adhikari, S, Ahmad, Z, Albright, CH, Alion, T, Amador, E, Anderson, J, Anderson, K, Andreopoulos, C, Andrews, M, Andrews, R, Anghel, I, Anjos, JD, Ankowski, A, Antonello, M, ArandaFernandez, A, Ariga, A, Ariga, T, Aristizabal, D, Arrieta-Diaz, E, Aryal, K, Asaadi, J, Asner, D, Athar, MS, Auger, M, Aurisano, A, Aushev, V, Autiero, D, Avila, M, Back, JJ, Bai, X, Baibussinov, B, Baird, M, Balantekin, AB, Baller, B, Ballett, P, Bambah, B, Bansal, M, Bansal, S, Barker, GJ, Barletta, WA, Barr, G, Barros, N, Bartoszek, L, Bashyal, A, Bass, M, Bay, F, Beacom, J, Behera, BR, Bellettini, G, Bellini, V, Beltramello, O, Benetti, PA, Bercellie, A, Bergevin, M, Berman, E, Berns, H, Bernstein, R, Bertolucci, S, Bhandari, B, Bhatnagar, V, Bhuyan, B, Bian, J, Biery, K, Bishai, M, Blackburn, T, Blake, A, Blaszczyk, FDM, Blaufuss, E, Bleakley, B, Blucher, E, Bocean, V, Boffelli, F, Boissevain, J, Bolognesi, S, Bolton, T, Bonesini, M, Boone, T, Booth, C, Bordoni, S, Borysova, M, Bourguille, B, Boyd, SB, Brailsford, D, Brandt, A, Bremer, J, Brice, S, Bromberg, C, Brooijmans, G, Brown, G, Brown, R, Brunetti, G, Bu, X, Buchanan, N, Budd, H, Bugg, B, Calafiura, P, Calligarich, E, Calvo, E, Camilleri, L, Campanelli, M, Cantini, C, Carls, B, Carr, R, Cascella, M, Castromonte, C, CatanoMur, E, Cavanna, F, Centro, S, CerveraVillanueva, A, Chandratre, VB, Chatterjee, A, Chattopadhyay, S, Chaussard, L, Chembra, S, Chen, H, Chen, K, Chen, M, Cherdack, D, Chi, C, Childress, S, Choubey, S, Choudhary, BC, Christodoulou, G, Christofferson, C, Church, E, Cianci, D, Cline, D, Coan, T, Cocco, A, Coelho, J, Cole, P, Collin, G, Conrad, JM, Convery, M, Corey, R, Corwin, L, Cranshaw, J, Crivelli, P, Cronin-Hennessy, D, Curioni, A, Cushing, J, Adams, DL, Dale, D, Das, SR, Davenne, T, Davies, GS, Davies, J, Dawson, J, De, K, deGouvea, A, deJong, JK, deJong, P, DeLurgio, P, Decowski, M, Delbart, A, Densham, C, Dharmapalan, R, Dhingra, N, DiLuise, S, Diamantopoulou, M, Diaz, JS, DiazBautista, G, Diwan, M, Djurcic, Z, Dolph, J, Drake, G, Duchesneau, D, Duvernois, M, Duyang, H, Dwyer, DA, Dye, S, Dytman, S, Eberly, B, Edgecock, R, Edmunds, D, Elliott, S, Elnimr, M, Emery, S, Endress, E, Eno, S, Ereditato, A, Escobar, CO, Evans, J, Falcone, A, Falk, L, Farbin, A, Farnese, C, Farzan, Y, Fava, A, Favilli, L, Felde, J, Felix, J, Fernandes, S, Fields, L, Finch, A, Fitton, M, Fleming, B, Forest, T, Fowler, J, Fox, W, Fried, J, Friedland, A, Fuess, S, Fujikawa, B, Gago, A, Gallagher, H, Galymov, S, Gamble, T, Gandhi, R, Garcia-Gamez, D, Gardiner, S, Garvey, G, Gehman, VM, Gendotti, A, Geronimo, GD, Ghag, C, Ghoshal, P, Gibin, D, Gil-Botella, I, Gill, R, Girardelli, D, Giri, A, Glavin, S, Goeldi, D, Golapinni, S, Gold, M, Gomes, RA, GomezCadenas, JJ, Goodman, MC, Gorbunov, D, Goswami, S, Graf, N, Graham, M, Gramelini, E, Gran, R, Grant, C, Grant, N, Greco, V, Greenlee, H, Greenler, L, Greenley, C, Groh, M, Grullon, S, Grundy, T, Grzelak, K, Guardincerri, E, Guarino, V, Guarnaccia, E, Guedes, GP, Guenette, R, Guglielmi, A, Habig, AT, Hackenburg, RW, Hackenburg, A, Hadavand, H, Haenni, R, Hahn, A, Haigh, MD, Haines, T, Hamernik, T, Handler, T, Hans, S, Harris, D, Hartnell, J, Hasegawa, T, Hatcher, R, Hatzikoutelis, A, Hays, S, Hazen, E, Headley, M, Heavey, A, Heeger, K, Heise, J, Hennessy, K, Hewes, J, Higuera, A, Hill, T, Himmel, A, Hogan, M, Holanda, P, Holin, A, Honey, W, Horikawa, S, Horton-Smith, G, Howard, B, Howell, J, Hurh, P, Huston, J, Hylen, J, Imlay, R, Insler, J, Introzzi, G, Ioanisyan, D, Ioannisian, A, Iwamoto, K, Izmaylov, A, Jackson, C, Jaffe, DE, James, C, James, E, Jediny, F, Jen, C, Jhingan, A, Jiménez, S, Jo, JH, Johnson, M, Johnson, R, Johnstone, J, Jones, BJ, Joshi, J, Jostlein, H, Jung, CK, Junk, T, Kaboth, A, Kadel, R, Kafka, T, Kalousis, L, Kamyshkov, Y, Karagiorgi, G, Karasavvas, D, Karyotakis, Y, Kaur, A, Kaur, P, Kayser, B, Kazaryan, N, Kearns, E, Keener, P, Kemboi, S, Kemp, E, Kettell, SH, Khabibullin, M, Khandaker, M, Khotjantsev, A, Kirby, B, Kirby, M, Klein, J, Kobilarcik, T, Kohn, S, Koizumi, G, Kopylov, A, Kordosky, M, Kormos, L, Kose, U, Kostelecky, A, Kramer, M, Kreslo, I, Kriske, R, Kropp, W, Kudenko, Y, Kudryavtsev, VA, Kulagin, S, Kumar, A, Kumar, G, Kumar, J, Kumar, L, Kutter, T, Laminack, A, Lande, K, Lane, C, Lang, K, Lanni, F, Learned, J, Lebrun, P, Lee, D, Lee, H, Lee, K, Lee, WM, LeiguideOliveira, MA, Li, Q, Li, S, Li, X, Li, Y, Li, Z, Libo, J, Lin, CS, Lin, S, Ling, J, Link, J, Liptak, Z, Lissauer, D, Littenberg, L, Littlejohn, B, Liu, Q, Liu, T, Lockwitz, S, Lockyer, N, Loew, T, Lokajicek, M, Long, K, Lopes, MDL, Lopez, JP, Losecco, J, Louis, W, Lowery, J, Luethi, M, Luk, K, Lundberg, B, Lundin, T, Luo, X, Lux, T, Lykken, J, Machado, AA, Macier, JR, Magill, S, Mahler, G, Mahn, K, Malek, M, Malhotra, S, Malon, D, Mammoliti, F, Mancina, S, Mandal, SK, Mandodi, S, Manly, SL, Mann, A, Marchionni, A, Marciano, W, Mariani, C, Maricic, J, Marino, A, Marshak, M, Marshall, C, Marshall, J, Marteau, J, Martin-Albo, J, Martinez, D, Matsuno, S, Matthews, J, Mauger, C, Mavrokoridis, K, Mayilyan, D, Mazzucato, E, McCauley, N, McCluskey, E, McConkey, N, McDonald, K, McFarland, KS, McGowan, AM, McGrew, C, McKeown, R, McNulty, D, McTaggart, R, Mefodiev, A, Mehrian, M, Mehta, P, Mei, D, Mena, O, Menary, S, Mendez, H, Menegolli, A, Meng, G, Meng, Y, Merritt, H, Mertins, D, Messier, M, Metcalf, W, Mewes, M, Meyer, H, Miao, T, Milincic, R, Miller, W, Mills, G, Mineev, O, Miranda, O, Mishra, CS, Mishra, SR, Mitrica, B, Mladenov, D, Mocioiu, I, Mohanta, R, Mokhov, N, Montanari, C, Montanari, D, Moon, J, Mooney, M, Moore, C, Morfin, J, Morgan, B, Morris, C, Morse, W, Moss, Z, Mossey, C, Moura, CA, Mousseau, J, Mualem, L, Muether, M, Mufson, S, Murphy, S, Musser, J, Musser, R, Nakajima, Y, Naples, D, Navarro, J, Navas, D, Nelson, J, Nessi, M, Newcomer, M, Ng, Y, Nichol, R, Nicholls, TC, Nikolics, K, Niner, E, Norris, B, Noto, F, Novakova, P, Novella, P, Nowak, J, Nunes, MS, O'Keeffe, H, Oldeman, R, Oliveira, R, Olson, T, Onishchuk, Y, Osta, J, Ovsjannikova, T, Page, B, Pakvasa, S, Pal, S, Palamara, O, Palazzo, A, Paley, J, Palomares, C, Pantic, E, Paolone, V, Papadimitriou, V, Park, J, Parke, S, Parsa, Z, Pascoli, S, Patterson, R, Patton, S, Patzak, T, Paulos, B, Paulucci, L, Pavlovic, Z, Pawloski, G, Peeters, S, Pennacchio, E, Perch, A, Perdue, GN, Periale, L, Perkin, JD, Pessard, H, Petrillo, G, Petti, R, Petukhov, A, Pietropaolo, F, Plunkett, R, Pordes, S, Potekhin, M, Potenza, R, Potukuchi, B, Poudyal, N, Prokofiev, O, Pruthi, N, Przewlocki, P, Pushka, D, Qian, X, Raaf, JL, Raboanary, R, Radeka, V, Radovic, A, Raffelt, G, Rakhno, I, Rakotondramanana, HT, Rakotondravohitra, L, Ramachers, YA, Rameika, R, Ramsey, J, Rappoldi, A, Raselli, G, Ratoff, P, Rebel, B, Regenfus, C, Reichenbacher, J, Reitzner, D, Remoto, A, Renshaw, A, Rescia, S, Richardson, M, Rielage, K, Riesselmann, K, Robinson, M, Rochester, L, Rodrigues, OB, Rodrigues, P, Roe, B, Rosen, M, Roser, RM, Ross-Lonergan, M, Rossella, M, Rubbia, A, Rubbia, C, Rucinski, R, RudolphvonRohr, C, Russell, B, Ruterbories, D, Saakyan, R, Sahu, N, Sala, P, Samios, N, Sanchez, F, Sanchez, M, Sands, B, Santana, S, Santorelli, R, Santucci, G, Saoulidou, N, Scaramelli, A, Schellman, H, Schlabach, P, Schmitt, R, Schmitz, D, Schneps, J, Scholberg, K, Schukraft, A, Schwehr, J, Segreto, E, Seibert, S, Sepulveda-Quiroz, JA, Sergiampietri, F, Sexton-Kennedy, L, Sgalaberna, D, Shaevitz, M, Shahi, J, Shahsavarani, S, Shanahan, P, Shankar, SU, Sharma, R, Sharma, RK, Shaw, T, Shrock, R, Shyrma, I, Simos, N, Sinev, G, Singh, I, Singh, J, Singh, V, Sinnis, G, Sippach, W, Smargianaki, D, Smy, M, Snider, E, Snopok, P, Sobczyk, J, Sobel, H, Soderberg, M, Solomey, N, Sondheim, W, Sorel, M, Sousa, A, Soustruznik, K, Spitz, J, Spooner, NJ, Stancari, M, Stancu, I, Stefan, D, Steiner, HM, Stewart, J, Stock, J, Stoica, S, Stone, J, Strait, J, Strait, M, Strauss, T, Striganov, S, Sulej, R, Sullivan, G, Sun, Y, Suter, L, Sutera, CM, Svoboda, R, Szczerbinska, B, Szelc, A, Söldner-Rembold, S, Talaga, R, Tamsett, M, Tariq, S, Tatar, E, Tayloe, R, Taylor, C, Taylor, D, Terao, K, Thiesse, M, Thomas, J, Thompson, LF, Thomson, M, Thorn, C, Thorpe, M, Tian, X, Tiedt, D, Timm, SC, Tonazzo, A, Tope, T, Topkar, A, Torres, FR, Torti, M, Tortola, M, Tortorici, F, Toups, M, Touramanis, C, Tripathi, M, Tropin, I, Tsai, Y, Tsang, KV, Tsenov, R, Tufanli, S, Tull, C, Turner, J, Tzanov, M, Tziaferi, E, Uchida, Y, Urheim, J, Usher, T, Vagins, M, Vahle, P, Valdiviesso, GA, Valerio, L, Vallari, Z, Valle, J, VanBerg, R, VandeWater, R, VanGemmeren, P, Varanini, F, Varner, G, Vasseur, G, Vaziri, K, Velev, G, Ventura, S, Verdugo, A, Viant, T, Vieira, TV, Vignoli, C, Vilela, C, Viren, B, Vrba, T, Wachala, T, Wahl, D, Wallbank, M, Walsh, N, Wang, B, Wang, H, Wang, L, Wang, T, Warburton, TK, Warner, D, Wascko, M, Waters, D, Watson, TB, Weber, A, Weber, M, Wei, W, Weinstein, A, Wells, D, Wenman, D, Wetstein, M, White, A, Whitehead, L, Whittington, D, Wilking, M, Willhite, J, Wilson, P, Wilson, RJ, Winslow, L, Wittich, P, Wojcicki, S, Wong, HH, Wood, K, Worcester, E, Worcester, M, Wu, S, Xin, T, Yanagisawa, C, Yang, S, Yang, T, Yarritu, K, Ye, J, Yeh, M, Yershov, N, Yonehara, K, Yu, B, Yu, J, Zalesak, J, Zalewska, A, Zamorano, B, Zang, L, Zani, A, Zavala, G, Zeller, G, Zhang, C, Zimmerman, ED, Zito, M, Zwaska, R, Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), DUNE, Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)
Subjects: Condensed Matter::Soft Condensed Matter, High Energy Physics - Experiment (hep-ex), Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], FOS: Physical sciences, High Energy Physics::Experiment, Instrumentation and Detectors (physics.ins-det), Nonlinear Sciences::Pattern Formation and Solitons, Physics::Geophysics, High Energy Physics - Experiment
Abstract: A description of the proposed detector(s) for DUNE at LBNF
Published: 2016

40. LUX-ZEPLIN (LZ) Conceptual Design Report

Author: Collaboration, TLZ, Akerib, DS, Akerlof, CW, Akimov, DY, Alsum, SK, Araújo, HM, Bai, X, Bailey, AJ, Balajthy, J, Balashov, S, Barry, MJ, Bauer, P, Beltrame, P, Bernard, EP, Bernstein, A, Biesiadzinski, TP, Boast, KE, Bolozdynya, AI, Boulton, EM, Bramante, R, Buckley, JH, Bugaev, VV, Bunker, R, Burdin, S, Busenitz, JK, Carels, C, Carlsmith, DL, Carlson, B, Carmona-Benitez, MC, Cascella, M, Chan, C, Cherwinka, JJ, Chiller, AA, Chiller, C, Craddock, WW, Currie, A, Cutter, JE, Cunha, JPD, Dahl, CE, Dasu, S, Davison, TJR, Viveiros, LD, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edberg, TK, Edwards, BN, Edwards, WR, Elnimr, MM, Emmet, WT, Faham, CH, Fiorucci, S, Ford, P, Francis, VB, Fu, C, Gaitskell, RJ, Gantos, NJ, Gehman, VM, Gerhard, RM, Ghag, C, Gilchriese, MGD, Gomber, B, Hall, CR, Harris, A, Haselschwardt, SJ, Hertel, SA, Hoff, MD, Holbrook, B, Holtom, E, Huang, DQ, Hurteau, TW, Ignarra, CM, Jacobsen, RG, Ji, W, Ji, X, Johnson, M, Ju, Y, Kamdin, K, Kazkaz, K, Khaitan, D, Khazov, A, Khromov, AV, Konovalov, AM, Korolkova, EV, Kraus, H, Krebs, HJ, Kudryavtsev, VA, Kumpan, AV, Kyre, S, Larsen, NA, Lee, C, Lenardo, BG, Lesko, KT, Liao, F-T, Lin, J, Lindote, A, Lippincott, WH, Liu, J, Liu, X, Lopes, MI, Lorenzon, W, Luitz, S, Majewski, P, Malling, DC, Manalaysay, AG, Manenti, L, Mannino, RL, Markley, DJ, Martin, TJ, Marzioni, MF, McKinsey, DN, Mei, D-M, Meng, Y, Miller, EH, Mock, J, Monzani, ME, Morad, JA, Murphy, ASJ, Nelson, HN, Neves, F, Nikkel, JA, O'Neill, FG, O'Dell, J, O'Sullivan, K, Olevitch, MA, Oliver-Mallory, KC, Palladino, KJ, Pangilinan, M, Patton, SJ, Pease, EK, Piepke, A, Powell, S, Preece, RM, Pushkin, K, Ratcliff, BN, Reichenbacher, J, Reichhart, L, Rhyne, C, Rodrigues, JP, Rose, HJ, Rosero, R, Saba, JS, Sarychev, M, Schnee, RW, Schubnell, MSG, Scovell, PR, Shaw, S, Shutt, TA, Silva, C, Skarpaas, K, Skulski, W, Solovov, VN, Sorensen, P, Sosnovtsev, VV, Stancu, I, Stark, MR, Stephenson, S, Stiegler, TM, Sumner, TJ, Sundarnath, K, Szydagis, M, Taylor, DJ, Taylor, W, Tennyson, BP, Terman, PA, Thomas, KJ, Thomson, JA, Tiedt, DR, To, WH, Tomás, A, Tripathi, M, Tull, CE, Tvrznikova, L, Uvarov, S, Va'vra, J, Grinten, MGDVD, Verbus, JR, Vuosalo, CO, Waldron, WL, Wang, L, Webb, RC, Wei, W-Z, While, M, White, DT, Whitis, TJ, Wisniewski, WJ, Witherell, MS, Wolfs, FLH, Woods, E, Woodward, D, Worm, SD, Yeh, M, Yin, J, Young, SK, and Zhang, C
Abstract: The design and performance of the LUX-ZEPLIN (LZ) detector is described as of March 2015 in this Conceptual Design Report. LZ is a second-generation dark-matter detector with the potential for unprecedented sensitivity to weakly interacting massive particles (WIMPs) of masses from a few GeV/c2 to hundreds of TeV/c2. With total liquid xenon mass of about 10 tonnes, LZ will be the most sensitive experiment for WIMPs in this mass region by the end of the decade. This report describes in detail the design of the LZ technical systems. Expected backgrounds are quantified and the performance of the experiment is presented. The LZ detector will be located at the Sanford Underground Research Facility in South Dakota. The organization of the LZ Project and a summary of the expected cost and current schedule are given.
Published: 2015

41. Inflammatory and neurodegenerative serum protein biomarkers increase sensitivity to detect clinical and radiographic disease activity in multiple sclerosis.

Author: Chitnis T, Qureshi F, Gehman VM, Becich M, Bove R, Cree BAC, Gomez R, Hauser SL, Henry RG, Katrib A, Lokhande H, Paul A, Caillier SJ, Santaniello A, Sattarnezhad N, Saxena S, Weiner H, Yano H, and Baranzini SE
Subjects: Humans, Female, Male, Adult, Middle Aged, Neurofilament Proteins blood, Blood Proteins analysis, Magnetic Resonance Imaging methods, Inflammation blood, Cohort Studies, Biomarkers blood, Multiple Sclerosis blood, Multiple Sclerosis diagnostic imaging, Proteomics methods
Abstract: The multifaceted nature of multiple sclerosis requires quantitative biomarkers that can provide insights related to diverse physiological pathways. To this end, proteomic analysis of deeply-phenotyped serum samples, biological pathway modeling, and network analysis were performed to elucidate inflammatory and neurodegenerative processes, identifying sensitive biomarkers of multiple sclerosis disease activity. Here, we evaluated the concentrations of > 1400 serum proteins in 630 samples from three multiple sclerosis cohorts for association with clinical and radiographic new disease activity. Twenty proteins were associated with increased clinical and radiographic multiple sclerosis disease activity for inclusion in a custom assay panel. Serum neurofilament light chain showed the strongest univariate correlation with gadolinium lesion activity, clinical relapse status, and annualized relapse rate. Multivariate modeling outperformed univariate for all endpoints. A comprehensive biomarker panel including the twenty proteins identified in this study could serve to characterize disease activity for a patient with multiple sclerosis., (© 2024. The Author(s).)
Published: 2024
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42. Clinical validation of a multi-protein, serum-based assay for disease activity assessments in multiple sclerosis.

Author: Chitnis T, Foley J, Ionete C, El Ayoubi NK, Saxena S, Gaitan-Walsh P, Lokhande H, Paul A, Saleh F, Weiner H, Qureshi F, Becich MJ, da Costa FR, Gehman VM, Zhang F, Keshavan A, Jalaleddini K, Ghoreyshi A, and Khoury SJ
Subjects: Humans, Magnetic Resonance Imaging, Blood Proteins, Gadolinium, Algorithms, Multiple Sclerosis
Abstract: An 18-protein multiple sclerosis (MS) disease activity (DA) test was validated based on associations between algorithm scores and clinical/radiographic assessments (N = 614 serum samples; Train [n = 426; algorithm development] and Test [n = 188; evaluation] subsets). The multi-protein model was trained based on presence/absence of gadolinium-positive (Gd+) lesions and was also strongly associated with new/enlarging T2 lesions, and active versus stable disease (composite of radiographic and clinical evidence of DA) with improved performance (p < 0.05) compared to the neurofilament light single protein model. The odds of having ≥1 Gd+ lesions with a moderate/high DA score were 4.49 times that of a low DA score, and the odds of having ≥2 Gd+ lesions with a high DA score were 20.99 times that of a low/moderate DA score. The MSDA Test was clinically validated with improved performance compared to the top-performing single-protein model and can serve as a quantitative tool to enhance the care of MS patients., Competing Interests: Declaration of Competing Interest Tanuja Chitnis has received compensation for consulting from Biogen, Novartis Pharmaceuticals, Roche Genentech, and Sanofi Genzyme, and has received research support from the National Institutes of Health, National MS Society, US Department of Defense, EMD Serono, I-Mab Biopharma, Mallinckrodt ARD, Novartis Pharmaceuticals, Octave Bioscience, Inc., Roche Genentech, and Tiziana Life Sciences. This research was conducted in part with the support of the Department of Defense through the Multiple Sclerosis Research Program under Award No. W81XWH-18-1-0648 (to T. Chitnis). John Foley has received research support from Biogen, Novartis, Adamas, Octave Bioscience, Inc., Genentech, and Mallinckrodt, has received speakers' honoraria and acted as a consultant for EMD Serono, Genzyme, Novartis, Biogen, and Genentech, has equity interest in Octave Bioscience, Inc., and is the founder of InterPro Bioscience. Carolina Ionete has received research support from Biogen, Serono, Genentech, NMSS, and the Department of Defense, and received compensation for advisory board activity from Sanofi-Genzyme. Nabil K. El Ayoubi has received support to attend scientific educational courses from Novartis, Merck Serono, Sanofi, Biologix, and has received speaker honoraria for scientific presentations on Multiple Sclerosis from Biologix, Sanofi, Merck Serono, and Novartis. Shrishti Saxena, Patricia Gaitan-Walsh, Anu Paul, and Fermisk Saleh have no disclosures. Hrishikesh Lokhande has received research support from the US Department of Defense and Octave Bioscience, Inc. Howard Weiner has received research support from the Department of Defense, Genentech, Inc., National Institutes of Health, National Multiple Sclerosis Society, Novartis, and Sanofi Genzyme. He has received compensation for consulting from Genentech, Inc., IM Therapeutics, IMAB Biopharma, MedDay Pharmaceuticals, Tiziana Life Sciences, and vTv Therapeutics. Ferhan Qureshi, Anisha Keshavan, Kian Jalaleddini, and Ati Ghoreyshi are employees of Octave Bioscience, Inc. Michael J. Becich, Fatima Rubio da Costa, Victor M. Gehman, and Fujun Zhang were employees of Octave Bioscience, Inc., at the time the study was completed. Samia J. Khoury has received compensation for scientific advisory board activity from Merck and Roche and for serving on IDMC for Biogen., (Copyright © 2023 The Authors. Published by Elsevier Inc. All rights reserved.)
Published: 2023
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43. Inflammatory and neurodegenerative serum protein biomarkers increase sensitivity to detect disease activity in multiple sclerosis.

Author: Chitnis T, Qureshi F, Gehman VM, Becich M, Bove R, Cree BAC, Gomez R, Hauser SL, Henry RG, Katrib A, Lokhande H, Paul A, Caillier SJ, Santaniello A, Sattarnezhad N, Saxena S, Weiner H, Yano H, and Baranzini SE
Abstract: Background/objectives: Serum proteomic analysis of deeply-phenotyped samples, biological pathway modeling and network analysis were performed to elucidate the inflammatory and neurodegenerative processes of multiple sclerosis (MS) and identify sensitive biomarkers of MS disease activity (DA)., Methods: Over 1100 serum proteins were evaluated in >600 samples from three MS cohorts to identify biomarkers of clinical and radiographic (gadolinium-enhancing lesions) new MS DA. Protein levels were analyzed and associated with presence of gadolinium-enhancing lesions, clinical relapse status (CRS), and annualized relapse rate (ARR) to create a custom assay panel., Results: Twenty proteins were associated with increased clinical and radiographic MS DA. Serum neurofilament light chain (NfL) showed the strongest univariate correlation with radiographic and clinical DA measures. Multivariate modeling significantly outperformed univariate NfL to predict gadolinium lesion activity, CRS and ARR., Discussion: These findings provide insight regarding correlations between inflammatory and neurodegenerative biomarkers and clinical and radiographic MS DA., Funding: Octave Bioscience, Inc (Menlo Park, CA).
Published: 2023
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44. Application of the small-angle approximation to ocean water types.

Author: Swanson NL, Billard BD, Gehman VM, and Gennaro TL
Abstract: The small-angle approximation to the radiative transport equation is applied to particle suspensions that emulate ocean water. A particle size distribution is constructed from polystyrene and glass spheres with the best available data for particle size distributions in the ocean. A volume scattering function is calculated from the Mie theory for the particles in water and in oil. The refractive-index ratios of particles in water and particles in oil are 1.19 and 1.01, respectively. The ratio 1.19 is comparable to minerals and nonliving diatoms in ocean water, and the ratio 1.01 is comparable to the lower limit for microbes in water. The point-spread functions are measured as a function of optical thickness for both water and oil mixtures and compared with the point-spread functions generated from the small-angle approximation. Our results show that, under conditions that emulate ocean water, the small-angle approximation is valid only for small optical thicknesses. Specifically, the approximation is valid only for optical thicknesses less than 3.
Published: 2001
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45. Limits of the small-angle approximation to the radiative transport equation.

Author: Swanson NL, Gehman VM, Billard BD, and Gennaro TL
Abstract: The small-angle approximation to the radiative transport equation is used extensively in imaging models in which the transport medium is optically thick. The small-angle approximation is generally considered valid when the particles are very large compared with the wavelength, when the refractive-index ratio of the particle to the medium is close to 1, and when the optical thickness is not too large. We report results showing the limits of the validity of the small-angle approximation as a function of particle size and concentration for a particle-to-medium fixed refractive-index ratio of 1.196. This refractive-index ratio is comparable with that of minerals or diatoms suspended in water.
Published: 2001
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